Photometric and Spectral Studies of the Group of Galactic Wolf-Rayet Stars. I. WN Sequence

被引：1
|
作者：
Kondratyeva, L. N. [1 ]
Reva, I. V. [1 ]
Denissyuk, E. K. [1 ]
Shomshekova, S. A. [1 ]
Aimanova, G. K. [1 ]
机构：
[1] VG Fesenkov Astrophys Inst AFIF, Alma Ata, Kazakhstan
来源：
ASTROPHYSICS | 2023年 / 66卷 / 04期
关键词：
variable stars; Wolf-Rayet (W-R) stars; photometry; spectrophotometry; COROTATING INTERACTION REGIONS; WIND; VARIABILITY; MASSES; CEPHEI;
D O I：
10.1007/s10511-024-09805-6
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Photometric and spectral observations of 11 Wolf-Rayet stars of the WN sequence were made at the AFIF during 2021-2022. Estimates of the brightness of objects in BVRc filters and the absolute fluxes of radiation in emission lines in this group are obtained on the basis of these observations. Changes in the brightness over a range of 0m.1-0m.15 are recorded for the stars WR 120, WR 151, and WR 152 in the WR I stars. Changes in the emission fluxes are detected in the spectra of several objects: WR 120, WR 128, and WR 145.
引用
收藏
页码：485 / 502
页数：18
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