Interactions in Massive Colliding Wind Binaries
There are observational difficulties determining dynamical masses of binary star components in the upper HR diagram both due to the scarcity of massive binary systems and spectral and photometric contamination produced by the strong wind outflows in these systems. We discuss how variable X-ray emi...
Main Author: | Michael F. Corcoran |
---|---|
Format: | Article |
Language: | English |
Published: |
The Korean Space Science Society
2012-03-01
|
Series: | Journal of Astronomy and Space Sciences |
Subjects: | |
Online Access: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2012/v29n1/OJOOBS_2012_v29n1_93.pdf |
Similar Items
-
Cygnus X-2: The descendant of an intermediate-mass X-ray binary
by: Podsiadlowski, P, et al.
Published: (2000) -
Multiwavelength Characterization of the High-mass X-Ray Binary Population of M33
by: Margaret Lazzarini, et al.
Published: (2023-01-01) -
POSYDON: A General-purpose Population Synthesis Code with Detailed Binary-evolution Simulations
by: Tassos Fragos, et al.
Published: (2023-01-01) -
Observations of Two Unusual Eclipsing Binaries, FN Cam and AG Vir
by: Avvakumova E. A., et al.
Published: (2014-12-01) -
The Major Role of Eccentricity in the Evolution of Colliding Pulsar-Stellar Winds
by: Maxim V. Barkov, et al.
Published: (2021-07-01)