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Concerning the occurrence of bow shocks around high-mass X-ray binaries

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PRIŠEGEN Michal

Druh Článek v odborném periodiku
Časopis / Zdroj Astronomy and Astrophysics
Fakulta / Pracoviště MU

Přírodovědecká fakulta

Citace
www https://ui.adsabs.harvard.edu/#abs/2019A&A...621A..37P/abstract
Doi http://dx.doi.org/10.1051/0004-6361/201832682
Klíčová slova proper motions; binaries: general; stars: early-type; stars: kinematics and dynamics; infrared: ISM
Popis 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.