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Browsing by Author Dačić, M.
Showing results 1 to 8 of 8
| Issue Date | Title | Author(s) | Type | Мp-cat. |
|---|---|---|---|---|
| 2009 | Activities of the Group for Astrophysical Spectroscopy 2005-2008 | Dimitrijević, Milan S.  ; Popović, L. Č.; Jevremović, D.; Dačić, M.; Jovanović, P.; Kovačević, A.; Simić, S.; Simić, Z.; Ilić, D.; Bon, E.;
Gavrilović, N.; Kovačević, J.; Milovanović, N.; Tankosić, D.; Stalevski, M.;
| Monograph | Mp. category will be shown later |
| 2008 | Electron-impact broadening of ionized chromium lines for Ap star atmospheres analysis | Dimitrijević, M. S.; Ryabchikova, T.; Simić, Z.; Popović, Luka Č.  ; Dačić, M. | Conference Paper | Mp. category will be shown later |
| 1999 | Proceedings of the 12th National Conference of Yugoslav Astronomers and International Workshop on the Development of Astronomical Databases, Beograd (Serbia), 19-21 Nov 1999. | Editorial works | Mp. category will be shown later | |
| 1999 | Proceedings of the 12th National Conference of Yugoslav Astronomers and International Workshop on the Development of Astronomical Databases, Beograd (Serbia), 19-21 Nov 1999. | Editorial works | Mp. category will be shown later | |
| 2004 | Some Spectroscopic Methods for Astrophysical Plasma Research | Popović, Luka Č. ; Dimitrijević, M. S. ; Mediavilla, E.; Danezis, E.; Lyratzi, E.; Bon, E. ; Ilić, Dragana ; Jovanović, P. ; Theodossiou, E.; Dačić, M. | Conference Paper | Mp. category will be shown later |
| 2005 | The flux ratio of [OIII]λ λ4959,5007 lines in Sy2: Comparison with theoretical calculations | Popović, Luka Č. ; Dimitrijević, M. S.; Bon, E.; Dačić, M. | Conference Paper | Mp. category will be shown later |
| 2007 | The flux ratio of the [OIII] λ λ 4959, 5007 Å lines in AGN | Dimitrijević, M.S.; Kovačević, J.; Popović, Luka Č. ; Dačić, M.; Ilić, Dragana | Conference Paper | Mp. category will be shown later |
| 2002 | The problem of the Fe II template in AGNs | Popović, Luka Č. ; Dimitrijević, M. S.; Dačić, M.; Kubičela, A. | Conference Paper | Mp. category will be shown later |