Publication details
Concerning the occurrence of bow shocks around high-mass X-ray binaries
| Authors | |
|---|---|
| Year of publication | 2019 |
| Type | Article in Periodical |
| Magazine / Source | Astronomy & Astrophysics |
| MU Faculty or unit | |
| Citation | |
| web | https://ui.adsabs.harvard.edu/#abs/2019A&A...621A..37P/abstract |
| Doi | https://doi.org/10.1051/0004-6361/201832682 |
| Keywords | proper motions; binaries: general; stars: early-type; stars: kinematics and dynamics; infrared: ISM |
| Description | Using the data from the space missions operating in the infrared and the astrometry from the Gaia satellite, we investigated the occurence of bow shocks around high-mass X-ray binaries. A number of circumstellar nebulae were found, however, genuine bow shocks were found to be rare, most likely due to low kinematical age of this class of objects - compared to the other types of runaway stars. |
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