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

Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F19%3A00109340" target="_blank" >RIV/00216224:14310/19:00109340 - isvavai.cz</a>
Výsledek na webu
<a href="https://ui.adsabs.harvard.edu/#abs/2019A&A...621A..37P/abstract" target="_blank" >https://ui.adsabs.harvard.edu/#abs/2019A&A...621A..37P/abstract</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201832682" target="_blank" >10.1051/0004-6361/201832682</a>

Jazyk výsledku
angličtina
Název v původním jazyce
Concerning the occurrence of bow shocks around high-mass X-ray binaries
Popis výsledku v původním jazyce
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.
Název v anglickém jazyce
Concerning the occurrence of bow shocks around high-mass X-ray binaries
Popis výsledku anglicky
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.

Rok uplatnění
2019
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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