ON THE EVOLUTION OF WOLF-RAYET STARS IN CLOSE BINARY SYSTEMS
The statistical study of the mass ratios of the components and eccentricities of close binary systems was made. Relations between these characteristics are obtained. Results of the analysis allows to conclude that at least 70 of all known WR+O binary systems (with orbital period P < 20d) where fo...
Main Authors: | A. M. Cherepashchuk, V. G. Karetnikov |
---|---|
Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2017-03-01
|
Series: | Odessa Astronomical Publications |
Online Access: | http://oap.onu.edu.ua/article/view/93010 |
Similar Items
-
Thermal structure of atmospheres of Wolf-Rayet stars
by: Oskinova L.M., et al.
Published: (1994-09-01) -
Newly Discovered Wolf–Rayet Stars in M31
by: Kathryn F. Neugent, et al.
Published: (2023-01-01) -
POLARIZATION ECLIPSE MODEL OF THE WOLF-RAYET BINARY V444 CYGNI WITH CONSTRAINS ON THE STELLAR RADII AND AN ESTIMATE OF THE WOLF-RAYET MASS-LOSS RATE
by: N. St-Louis, et al.
Published: (2017-07-01) -
Probing the Stellar Wind of the Wolf–Rayet Star in IC 10 X-1
by: Sayantan Bhattacharya, et al.
Published: (2023-01-01) -
INTERPRETATION AND SOLUTION OF THE LIGHT CURVE OF THE WOLF-RAYET ECLIPSING BINARY CQ CEP
by: T. A. Kartasheva, et al.
Published: (2017-07-01)