TY  - JOUR
AU  - Tančić, Pavle
AU  - Dušanić, Slađana
AU  - Erić, Suzana
PY  - 2023
UR  - https://cer.ihtm.bg.ac.rs/handle/123456789/6185
AB  - The grossular garnet from rodingite-type rock from the Suva Česma area in western Serbia is characterized with its weak anisotropic nature. Because its anisotropy could indicate a non-cubic lower symmetry, SEM-EDS and Rietveld powder refinement methods were used. The SEM-EDS results have shown that the garnet has a (Ca3.00Mn0.01)3.01(Al1.82Fe0.15Ti0.02)1.99(Si2.97Al0.03)3.00O12 chemical composition (i.e., Grs91Adr08), which can be more specifically explained as ferric iron containing grossular. The next step further used Rietveld powder refinements of the various crystal structures in the Ia‾3d, R‾3c, R‾3, I41/a, Fddd, C2/c, and I‾1 space groups as well as a single mixture, which was followed by a comparative analysis of the R-values, site occupancy factors, and bond lengths and angles. The synthesis of these results showed both that the studied grossular garnet is not cubic and that it crystallized in the disordered Fddd space group with the final RB = 5.29% and RF = 1.75%. It was presumed that the grossular formed at temperatures between 150 and ~600 °C.
PB  - MDPI
T2  - Powders
T1  - Orthorhombic Crystal Structure of Grossular Garnet (Suva Česma, Western Serbia): Evidence from the Rietveld Refinement
VL  - 2
IS  - 2
SP  - 387
EP  - 402
DO  - 10.3390/powders2020023
ER  - 

@article{
author = "Tančić, Pavle and Dušanić, Slađana and Erić, Suzana",
year = "2023",
abstract = "The grossular garnet from rodingite-type rock from the Suva Česma area in western Serbia is characterized with its weak anisotropic nature. Because its anisotropy could indicate a non-cubic lower symmetry, SEM-EDS and Rietveld powder refinement methods were used. The SEM-EDS results have shown that the garnet has a (Ca3.00Mn0.01)3.01(Al1.82Fe0.15Ti0.02)1.99(Si2.97Al0.03)3.00O12 chemical composition (i.e., Grs91Adr08), which can be more specifically explained as ferric iron containing grossular. The next step further used Rietveld powder refinements of the various crystal structures in the Ia‾3d, R‾3c, R‾3, I41/a, Fddd, C2/c, and I‾1 space groups as well as a single mixture, which was followed by a comparative analysis of the R-values, site occupancy factors, and bond lengths and angles. The synthesis of these results showed both that the studied grossular garnet is not cubic and that it crystallized in the disordered Fddd space group with the final RB = 5.29% and RF = 1.75%. It was presumed that the grossular formed at temperatures between 150 and ~600 °C.",
publisher = "MDPI",
journal = "Powders",
title = "Orthorhombic Crystal Structure of Grossular Garnet (Suva Česma, Western Serbia): Evidence from the Rietveld Refinement",
volume = "2",
number = "2",
pages = "387-402",
doi = "10.3390/powders2020023"
}

Tančić, P., Dušanić, S.,& Erić, S.. (2023). Orthorhombic Crystal Structure of Grossular Garnet (Suva Česma, Western Serbia): Evidence from the Rietveld Refinement. in Powders
MDPI., 2(2), 387-402.
https://doi.org/10.3390/powders2020023

Tančić P, Dušanić S, Erić S. Orthorhombic Crystal Structure of Grossular Garnet (Suva Česma, Western Serbia): Evidence from the Rietveld Refinement. in Powders. 2023;2(2):387-402.
doi:10.3390/powders2020023 .

Tančić, Pavle, Dušanić, Slađana, Erić, Suzana, "Orthorhombic Crystal Structure of Grossular Garnet (Suva Česma, Western Serbia): Evidence from the Rietveld Refinement" in Powders, 2, no. 2 (2023):387-402,
https://doi.org/10.3390/powders2020023 . .

TY  - DATA
AU  - Tančić, Pavle
AU  - Dušanić, Slađana
AU  - Erić, Suzana
PY  - 2023
UR  - https://cer.ihtm.bg.ac.rs/handle/123456789/6977
AB  - Table S1. Profile parameters for the studied space groups without constraints.; Table S2. Unit cell dimensions and quantitative contents of garnet and chlorite for the studied space groups without constraints. Calculated 4 × c0/a0 parameters and distortion angles (α) for the rhombohedral R‾3c and R‾3 s.g.’s, and specific geometry–mathematical transformations [5,6] of the crystallographic axes within Ia‾3d, R‾3c, R‾3, Fddd, C2/c, and I‾1 s.g.’s are also presented.; Table S3. Calculated Al sof’s (in %) and selected Si-O, Y-O, and Ca-O distances (in Å) for the studied space groups without constraints.; Table S4. Profile parameters for the studied space groups with constraints.; Table S5. Unit cell dimensions and quantitative contents of garnet and chlorite for the studied space groups with constraints. Calculated 4 × c0/a0 parameters and distortion angles (α) for the rhombohedral R‾3c and R‾3 s.g.’s, and specific geometry–mathematical transformations [5,6] of the crystallographic axes within Ia‾3d, R‾3c, R‾3, Fddd, C2/c, and I‾1 s.g.’s, are also presented.; Table S6. Calculated Al sof’s (in %) and selected Si–O, Y–O, and Ca–O distances (in Å) for the studied space groups with constraints.; Table S7. Selected distances (in Å) and angles (in °) for the orthorhombic Fddd space group (withouta and withb constraints).; Table S8. Selected distances among the studied cation sites (in Å) for the orthorhombic Fddd space group (withouta and withb constraints).; Figure S1. Final Rietveld plot for the Ia‾3d space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite.; Figure S2. Final Rietveld plot for the R‾3c space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars: upper row: garnet; lower row: chlorite; Figure S3. Final Rietveld plot for the Fddd space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row-garnet; lower row-chlorite; Figure S4. Final Rietveld plot for the C2/c space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S5. Final Rietveld plot for the I‾1 space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S6. Final Rietveld plot for the R‾3 space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S7. Final Rietveld plot for the I41/a space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S8. Final Rietveld plot for the Ia‾3d space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S9. Final Rietveld plot for the R‾3c space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S10. Final Rietveld plot for the Fddd space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S11. Final Rietveld plot for the C2/c space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S12. Final Rietveld plot for the I‾1 space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S13. Final Rietveld plot for the R‾3 space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S14. Final Rietveld plot for the I41/a space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite.
PB  - MDPI, Basel, Switzerland
T2  - Powders
T1  - Supplementary Materials for: "Orthorhombic crystal structure of grossular garnet (Suva Česma, Western Serbia): Evidence from the Rietveld refinement"
UR  - https://hdl.handle.net/21.15107/rcub_cer_6977
ER  - 

@misc{
author = "Tančić, Pavle and Dušanić, Slađana and Erić, Suzana",
year = "2023",
abstract = "Table S1. Profile parameters for the studied space groups without constraints.; Table S2. Unit cell dimensions and quantitative contents of garnet and chlorite for the studied space groups without constraints. Calculated 4 × c0/a0 parameters and distortion angles (α) for the rhombohedral R‾3c and R‾3 s.g.’s, and specific geometry–mathematical transformations [5,6] of the crystallographic axes within Ia‾3d, R‾3c, R‾3, Fddd, C2/c, and I‾1 s.g.’s are also presented.; Table S3. Calculated Al sof’s (in %) and selected Si-O, Y-O, and Ca-O distances (in Å) for the studied space groups without constraints.; Table S4. Profile parameters for the studied space groups with constraints.; Table S5. Unit cell dimensions and quantitative contents of garnet and chlorite for the studied space groups with constraints. Calculated 4 × c0/a0 parameters and distortion angles (α) for the rhombohedral R‾3c and R‾3 s.g.’s, and specific geometry–mathematical transformations [5,6] of the crystallographic axes within Ia‾3d, R‾3c, R‾3, Fddd, C2/c, and I‾1 s.g.’s, are also presented.; Table S6. Calculated Al sof’s (in %) and selected Si–O, Y–O, and Ca–O distances (in Å) for the studied space groups with constraints.; Table S7. Selected distances (in Å) and angles (in °) for the orthorhombic Fddd space group (withouta and withb constraints).; Table S8. Selected distances among the studied cation sites (in Å) for the orthorhombic Fddd space group (withouta and withb constraints).; Figure S1. Final Rietveld plot for the Ia‾3d space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite.; Figure S2. Final Rietveld plot for the R‾3c space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars: upper row: garnet; lower row: chlorite; Figure S3. Final Rietveld plot for the Fddd space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row-garnet; lower row-chlorite; Figure S4. Final Rietveld plot for the C2/c space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S5. Final Rietveld plot for the I‾1 space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S6. Final Rietveld plot for the R‾3 space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S7. Final Rietveld plot for the I41/a space group without constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S8. Final Rietveld plot for the Ia‾3d space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S9. Final Rietveld plot for the R‾3c space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S10. Final Rietveld plot for the Fddd space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S11. Final Rietveld plot for the C2/c space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S12. Final Rietveld plot for the I‾1 space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S13. Final Rietveld plot for the R‾3 space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite; Figure S14. Final Rietveld plot for the I41/a space group with constraints. Observed intensities (Yobs) were presented with red color, calculated intensities (Ycalc) were presented with black color, and differences between observed and calculated intensities (Yobs-Ycalc) were presented with blue color. Reflection (Bragg) positions were presented with green vertical bars; upper row: garnet; lower row: chlorite.",
publisher = "MDPI, Basel, Switzerland",
journal = "Powders",
title = "Supplementary Materials for: "Orthorhombic crystal structure of grossular garnet (Suva Česma, Western Serbia): Evidence from the Rietveld refinement"",
url = "https://hdl.handle.net/21.15107/rcub_cer_6977"
}

Tančić, P., Dušanić, S.,& Erić, S.. (2023). Supplementary Materials for: "Orthorhombic crystal structure of grossular garnet (Suva Česma, Western Serbia): Evidence from the Rietveld refinement". in Powders
MDPI, Basel, Switzerland..
https://hdl.handle.net/21.15107/rcub_cer_6977

Tančić P, Dušanić S, Erić S. Supplementary Materials for: "Orthorhombic crystal structure of grossular garnet (Suva Česma, Western Serbia): Evidence from the Rietveld refinement". in Powders. 2023;.
https://hdl.handle.net/21.15107/rcub_cer_6977 .

Tančić, Pavle, Dušanić, Slađana, Erić, Suzana, "Supplementary Materials for: "Orthorhombic crystal structure of grossular garnet (Suva Česma, Western Serbia): Evidence from the Rietveld refinement"" in Powders (2023),
https://hdl.handle.net/21.15107/rcub_cer_6977 .

TY  - JOUR
AU  - Životić, Dragana
AU  - Cvetković, Olga
AU  - Vulić, Predrag J.
AU  - Gržetić, Ivan
AU  - Simić, Vladimir
AU  - Ilijević, Konstantin
AU  - Dojčinović, Biljana
AU  - Erić, Suzana
AU  - Radić, Bogdan
AU  - Stojadinović, Sanja
AU  - Trifunović, Snežana S.
PY  - 2019
UR  - https://cer.ihtm.bg.ac.rs/handle/123456789/3353
AB  - A geochemical and mineralogical study was performed on lignite samples from the Upper Miocene Kovin deposit, hosting three coal seams. The Kovin lignite is characterized by high moisture content, medium to high ash yield, medium to high sulphur content and a relatively low gross and net calorific value. The mineralogical composition, and major and trace element contents were determined by X-ray diffraction, scanning electron microscopy with energy dispersive X-ray spectroscopy (SEM-EDS) analyses, and inductively coupled plasma optical emission spectrometry (ICP-OES). The most abundant minerals in all lignite samples from the three coal seams are clays (illite/smectite), silicates (quartz, plagioclase), sulphates (gypsum/anhydrite) and carbonate (calcite). The other iron-rich minerals are sulphides, oxides and hydroxides (pyrite, mag-netite, haematite, and limonite). In general, mineral matter in the matrix coal consists of illite/ smectite and quartz, while xylite-rich coals, apart from illite/smectite, have a higher content of sulphates and Fe-oxide/hydroxide minerals. The lignite from the Kovin deposit is enriched in As, Cd, Co, Cr, Cu, Ga, Li, Mn, Mo, Ni, Pb, V, Zn, Gd, Tb, Er and Lu in comparison with the Clarke values for brown coals. The statistical analysis of bulk compositional data shows inorganic affinity for the majority of the major and trace elements and possible association with pyrite, illite/ smectite and calcite.
PB  - Institut za Geoloska Istrazivanja
T2  - Geologia Croatica
T1  - Distribution of major and trace elements in the Kovin lignite (Serbia)
VL  - 72
IS  - 1
SP  - 51
EP  - 79
DO  - 10.4154/gc.2019.06
ER  - 

@article{
author = "Životić, Dragana and Cvetković, Olga and Vulić, Predrag J. and Gržetić, Ivan and Simić, Vladimir and Ilijević, Konstantin and Dojčinović, Biljana and Erić, Suzana and Radić, Bogdan and Stojadinović, Sanja and Trifunović, Snežana S.",
year = "2019",
abstract = "A geochemical and mineralogical study was performed on lignite samples from the Upper Miocene Kovin deposit, hosting three coal seams. The Kovin lignite is characterized by high moisture content, medium to high ash yield, medium to high sulphur content and a relatively low gross and net calorific value. The mineralogical composition, and major and trace element contents were determined by X-ray diffraction, scanning electron microscopy with energy dispersive X-ray spectroscopy (SEM-EDS) analyses, and inductively coupled plasma optical emission spectrometry (ICP-OES). The most abundant minerals in all lignite samples from the three coal seams are clays (illite/smectite), silicates (quartz, plagioclase), sulphates (gypsum/anhydrite) and carbonate (calcite). The other iron-rich minerals are sulphides, oxides and hydroxides (pyrite, mag-netite, haematite, and limonite). In general, mineral matter in the matrix coal consists of illite/ smectite and quartz, while xylite-rich coals, apart from illite/smectite, have a higher content of sulphates and Fe-oxide/hydroxide minerals. The lignite from the Kovin deposit is enriched in As, Cd, Co, Cr, Cu, Ga, Li, Mn, Mo, Ni, Pb, V, Zn, Gd, Tb, Er and Lu in comparison with the Clarke values for brown coals. The statistical analysis of bulk compositional data shows inorganic affinity for the majority of the major and trace elements and possible association with pyrite, illite/ smectite and calcite.",
publisher = "Institut za Geoloska Istrazivanja",
journal = "Geologia Croatica",
title = "Distribution of major and trace elements in the Kovin lignite (Serbia)",
volume = "72",
number = "1",
pages = "51-79",
doi = "10.4154/gc.2019.06"
}

Životić, D., Cvetković, O., Vulić, P. J., Gržetić, I., Simić, V., Ilijević, K., Dojčinović, B., Erić, S., Radić, B., Stojadinović, S.,& Trifunović, S. S.. (2019). Distribution of major and trace elements in the Kovin lignite (Serbia). in Geologia Croatica
Institut za Geoloska Istrazivanja., 72(1), 51-79.
https://doi.org/10.4154/gc.2019.06

Životić D, Cvetković O, Vulić PJ, Gržetić I, Simić V, Ilijević K, Dojčinović B, Erić S, Radić B, Stojadinović S, Trifunović SS. Distribution of major and trace elements in the Kovin lignite (Serbia). in Geologia Croatica. 2019;72(1):51-79.
doi:10.4154/gc.2019.06 .

Životić, Dragana, Cvetković, Olga, Vulić, Predrag J., Gržetić, Ivan, Simić, Vladimir, Ilijević, Konstantin, Dojčinović, Biljana, Erić, Suzana, Radić, Bogdan, Stojadinović, Sanja, Trifunović, Snežana S., "Distribution of major and trace elements in the Kovin lignite (Serbia)" in Geologia Croatica, 72, no. 1 (2019):51-79,
https://doi.org/10.4154/gc.2019.06 . .

TY  - JOUR
AU  - Erić, Suzana
AU  - Tančić, Pavle
AU  - Đurić, Stevan
PY  - 1994
UR  - https://cer.ihtm.bg.ac.rs/handle/123456789/6182
AB  - Korund iz distensko silimanitskog škriljca lokalnosti Bobološ je detaljnije mineraloško-kristalografski ispitan pomoću nekoliko metoda. Dobijeno je učešće korunda od oko 15 %, čime je ova stena postala značajna kao sirovina za aluminijske opeke. Takođe je ispitan plavi korund safirskog tipa koji se ovde javlja pri čemu je dobijena sledeća jedinična ćelija: a0=4,7600 /8/ A, c0=12,98 /1/ A i V0=254,6 /4/ A3.
PB  - Geoinstitut
T2  - Radovi
T1  - Корунд из дистенско-силиманитског шкриљца Боболош-Брза Паланка
VL  - 30
SP  - 65
EP  - 71
UR  - https://hdl.handle.net/21.15107/rcub_cer_6182
ER  - 

@article{
author = "Erić, Suzana and Tančić, Pavle and Đurić, Stevan",
year = "1994",
abstract = "Korund iz distensko silimanitskog škriljca lokalnosti Bobološ je detaljnije mineraloško-kristalografski ispitan pomoću nekoliko metoda. Dobijeno je učešće korunda od oko 15 %, čime je ova stena postala značajna kao sirovina za aluminijske opeke. Takođe je ispitan plavi korund safirskog tipa koji se ovde javlja pri čemu je dobijena sledeća jedinična ćelija: a0=4,7600 /8/ A, c0=12,98 /1/ A i V0=254,6 /4/ A3.",
publisher = "Geoinstitut",
journal = "Radovi",
title = "Корунд из дистенско-силиманитског шкриљца Боболош-Брза Паланка",
volume = "30",
pages = "65-71",
url = "https://hdl.handle.net/21.15107/rcub_cer_6182"
}

Erić, S., Tančić, P.,& Đurić, S.. (1994). Корунд из дистенско-силиманитског шкриљца Боболош-Брза Паланка. in Radovi
Geoinstitut., 30, 65-71.
https://hdl.handle.net/21.15107/rcub_cer_6182

Erić S, Tančić P, Đurić S. Корунд из дистенско-силиманитског шкриљца Боболош-Брза Паланка. in Radovi. 1994;30:65-71.
https://hdl.handle.net/21.15107/rcub_cer_6182 .

Erić, Suzana, Tančić, Pavle, Đurić, Stevan, "Корунд из дистенско-силиманитског шкриљца Боболош-Брза Паланка" in Radovi, 30 (1994):65-71,
https://hdl.handle.net/21.15107/rcub_cer_6182 .