Researchers
Dimitrijević, Milan
Results 541-560 of 618
| Issue Date | Title | Author(s) | Type | Мp-cat. |
|---|---|---|---|---|
| 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 |
| 2003 | On the stark broadening of neutral germanium spectral lines | Dimitrijevic, Milan S ; Jovanovic, Predrag P ; Simic, Zoran J | Conference Paper | Mp. category will be shown later |
| 2003 | Kr II transition probabilities for analysis of trace element lines in high resolution stellar spectra | Dimitrijević, Milan S. ; Milosavljević, Vladimir M.; Djeniže, Stevan I. | Monograph | Mp. category will be shown later |
| 2003 | Transition probabilities in KrII and KrIII spectra | Djenize, Stevan; Milosavljevic, Vladimir M ; Dimitrijevic, Milan S | Article | 22M22 |
| 2003 | Correlation between X-ray continuum and Fe Kα line variation due to microlensing | Jovanović, P. ; Popović, Luka Č. ; Dimitrijević, M. S. | Conference Paper | Mp. category will be shown later |
| 2003 | Influence of stark broadening within BeIII spectral series | Dimitrijevic, Milan S ; Dacic, Miodrag D; Cvetkovic, Zorica D; Sahal-Brechot, Sylvie | Conference Paper | Mp. category will be shown later |
| 2003 | Stark broadening of spectral line shapes (on the French-Serbian collaboration) | Dimitrijevic, Milan S ; Sahal-Brechot, Sylvie | Article | 22M22 |
| 2003 | Stark broadening of AgI spectral lines | Dimitrijevic, Milan S ; Sahal-Brechot, Sylvie | Article | 21aM21a |
| 2003 | Stark broadening of neutral germanium spectral lines in astrophysical plasma | Dimitrijevic, Milan S ; Jovanovic, Predrag P | Conference Paper | Mp. category will be shown later |
| 2003 | Stark broadening of F III lines in stellar plasma | Simić, Zoran ; Dimitrijević, Milan S. ; Popović, Luka Č. | Monograph | Mp. category will be shown later |
| 2003 | Transition probabilities in Kr III spectrum, of interest for high resolution stellar spectra analysis | Djenize, Stevan; Milosavljevic, Vladimir M ; Dimitrijevic, Milan S | Conference Paper | Mp. category will be shown later |
| 2003 | Importance of collisions with charged particles for stellar UV line shapes: Cd III | Milovanović, N.; Dimitrijević, M. S. ; Popović, Luka Č. ; Simić, Z. | Conference Paper | Mp. category will be shown later |
| 2003 | Stark broadening of neutral germanium spectral lines | Dimitrijevic, Milan S ; Jovanovic, Predrag P ; Simic, Zoran J | Article | 21M21 |
| 2003 | Influence of chemi-ionization and chemi-recombination processes on the population of hydrogen Rydberg states in atmospheres of late type dwarfs | Mihajlov, A. A.; Jevremovic, D.; Hauschildt, P.; Dimitrijević, M. S. ; Ignjatović, Ljubiša ; Alard, F. | Article | 21M21 |
| 2003 | On the influence of Stark broadening on Si I lines in stellar atmospheres | Dimitrijević, M. S. ; Ryabchikova, T.; Popović, Luka Č. ; Shulyak, D.; Tsymbal, V. | Article | 21M21 |
| 2003 | Stark broadening of F III lines in stellar plasma | Simić, Z.; Dimitrijević, M. S. ; Popović, Luka Č. | Conference Paper | Mp. category will be shown later |
| 2003 | VizieR Online Data Catalog: Zr II & III electron-impact broadening parameters (Popovic+, 2001) | Popovic, L. C. ; Milovanovic, N. ; Dimitrijevic, M. S. | Dataset | Mp. category will be shown later |
| 2003 | Stark broadening of spectral lines of multicharged ions of astrophysical interest. XXIII. BeIII | Dimitrijevic, Milan S ; Dacic, Miodrag D; Cvetkovic, Zorica D; Sahal-Brechot, Sylvie | Article | 21M21 |
| 2003 | Symmetrical chemi-ionization and chemi-recombination processes in low-temperature layers of helium-rich DB white dwarf atmospheres | Mihajlov, A. A.; Ignjatović, Ljubiša ; Dimitrijević, M. S. ; Djurić, Z. | Article | 21aM21a |
| 2003 | VizieR Online Data Catalog: Co III electron-impact broadening parameters (Tankosic+, 2003) | Tankosic, D.; Popovic, L. C. ; Dimitrijevic, M. S. | Dataset | Mp. category will be shown later |