Milosavljević, V., Djeniže, S. (2002) Ion contribution to the astrophysical important 447.15, 587.56 and 667.82 nm He I spectral lines broadening. Astronomy & Astrophysics, 393 (2). 721-726 doi:10.1051/0004-6361:20021174

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Reference Type	Journal (article/letter/editorial)
Title	Ion contribution to the astrophysical important 447.15, 587.56 and 667.82 nm He I spectral lines broadening
Journal	Astronomy & Astrophysics
Authors	Milosavljević, V.		Author
Authors	Djeniže, S.		Author
Year	2002 (October)	Volume	393
Issue	2
Publisher	EDP Sciences
DOI	doi:10.1051/0004-6361:20021174Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	3459582	Long-form Identifier	mindat:1:5:3459582:6
GUID	0
Full Reference	Milosavljević, V., Djeniže, S. (2002) Ion contribution to the astrophysical important 447.15, 587.56 and 667.82 nm He I spectral lines broadening. Astronomy & Astrophysics, 393 (2). 721-726 doi:10.1051/0004-6361:20021174
Plain Text	Milosavljević, V., Djeniže, S. (2002) Ion contribution to the astrophysical important 447.15, 587.56 and 667.82 nm He I spectral lines broadening. Astronomy & Astrophysics, 393 (2). 721-726 doi:10.1051/0004-6361:20021174
In	(2002, October) Astronomy & Astrophysics Vol. 393 (2) EDP Sciences

	Milosavljević, V., Djeniže, S. (2002) Ion contribution to the astrophysical important 388.86, 471.32 and 501.56 nm He I spectral lines broadening. New Astronomy, 7. 543-551 doi:10.1016/s1384-1076(02)00177-x
	Milosavljević, V., Djeniže, S. (2003) Ion contribution to the prominent Ne I, Ar I and Kr I spectral line broadening. Astronomy & Astrophysics, 398 (3). 1179-1184 doi:10.1051/0004-6361:20021654
	Milosavljević, V., Djeniže, S. (2003) Astrophysical plasma diagnostics through analysis of $\ion{Ar}{I}$ line shape characteristics. Astronomy & Astrophysics, 405 (2). 397-403 doi:10.1051/0004-6361:20030612
	*Milosavljević, V, Djeniže, S (2002) Ion contribution to the NeI spectral lines broadening. Physics Letters A, 305. 70-74 doi:10.1016/s0375-9601(02)01354-3*
	*Djeniže, S., Milosavljević, V., Dimitrijević, M. S. (2002) Stark shifts and transition probabilities in the Ne spectrum. Astronomy & Astrophysics, 382 (1). 359-367 doi:10.1051/0004-6361:20011549*
	*Simić, Z., Dimitrijević, M. S., Milovanović, N., Sahal-Bréchot, S. (2005) Stark broadening of Cd I spectral lines. Astronomy & Astrophysics, 441 (1). 391-393 doi:10.1051/0004-6361:20052701*
	*Milosavljević, V., Djeniže, S. (2001) On the Stark broadening of the He I 447.1 nm spectral line. The European Physical Journal D, 15. 99-104 doi:10.1007/s100530170187*
	*Djeniže, S., Bukvić, S., Mišković, D. (2001) Stark widths and shifts of triply ionized argon spectral lines. Astronomy & Astrophysics, 367 (2). 737-740 doi:10.1051/0004-6361:20000453*
	Djeniže, S., Srećković, A., Jelisavčić, M., Bukvić, S. (2002) Experimental Stark widths and shifts of triply ionized sulfur spectral lines. Astronomy & Astrophysics, 389 (3). 1086-1089 doi:10.1051/0004-6361:20020717
	*Milosavljević, V., Djeniže, S. (1998) Measured Stark widths and shifts of NII, NIII and NIV spectral lines. Astronomy and Astrophysics Supplement Series, 128. 197-201 doi:10.1051/aas:1998135*
	Djeniže, S., Milosavljević, V. (1998) Measured Stark widths and shifts of several N III spectral lines: Temperature dependence. Astronomy and Astrophysics Supplement Series, 131. 355-359 doi:10.1051/aas:1998272

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Milosavljević, V., Djeniže, S. (2002) Ion contribution to the astrophysical important 447.15, 587.56 and 667.82 nm He I spectral lines broadening. Astronomy & Astrophysics, 393 (2). 721-726 doi:10.1051/0004-6361:20021174

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