2020MNRAS.496.5584M

Query : 2020MNRAS.496.5584M

2020MNRAS.496.5584M - Mon. Not. R. Astron. Soc., 496, 5584-5590 (2020/August-3)

Stark broadening of Co II spectral lines in hot stars and white dwarf spectra.

MAJLINGER Z., DIMITRIJEVIC M.S. and SRECKOVIC V.A.

Abstract (from CDS):

Stark full widths at half-maximum for 46 Co II multiplets have been calculated using modified semi-empirical method. The obtained results have been used to demonstrate the importance of Stark broadening mechanism in DA and DB white dwarf and A star atmospheres. With the obtained results we also test possibility of using some approximate methods of Stark width calculations developed on the basis of regularities and systematic trends.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): atomic data - atomic processes - line: formation

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 V* KZ Cam a2* 03 38 19.7334959304 +56 55 57.775389816 7.589 6.176 6.282     B9p 82 0
2 HD 89490 PM* 10 19 32.3443779090 -05 06 22.132076553   7.271 6.361     K0IV 28 0
3 V* V2200 Cyg a2* 21 01 14.3203959696 +43 43 18.402894444   7.60 7.68     B9p 131 0
4 V* BI Mic a2* 21 26 03.8683509936 -29 55 48.145296468   9.10 8.81     ApSrEu 87 0
5 V* BD Ind a2* 21 56 56.6970333720 -61 50 46.320856080   7.42 7.19     ApSrEuCr 66 0

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