Fundamental parameters of some B-type stars using NOAO Indo-U. S. Library

被引:1
|
作者
Shokry, A. [1 ,2 ]
Nouh, M., I [1 ]
Saad, S. M. [1 ,2 ]
Helmy, I [1 ]
机构
[1] Natl Res Inst Astron & Geophys NRIAG, Astron Dept, Cairo 11421, Egypt
[2] Kottamia Ctr Sci Excellence Astron & Space Sci, KCScE, STDF, ASRT, Cairo, Egypt
基金
美国国家科学基金会;
关键词
Field B -stars; BCD method; Fundamental parameters; ROTATIONAL VELOCITIES; EFFECTIVE TEMPERATURES; STELLAR ROTATION; BLUE; SUPERGIANTS; CALIBRATION; SPECTRA; RADII; FIELD;
D O I
10.1016/j.newast.2022.101780
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this article, we present a spectroscopic analysis of 83 field B-type stars from NOAO Indo-U.S. Library. We calculated the fundamental parameters such as effective temperatures, surface gravities, and rotational velocities using Barbier-Chalonge-Divan (BCD) method and line blanketed LTE/NLTE model atmospheres. The projected rotational velocities were estimated by fitting the Mg II4481 angstrom line profile with theoretical lines calculated from LTE/NLTE models. The evolutionary masses for the program stars are estimated using the evolutionary models. In most of the cases, the present study gives fair agreement with earlier investigations and is even more accurate in some cases.
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页数:10
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