OB runaway stars originating in the Vel OB1 association

Context. OB runaway stars are massive stars moving through interstellar space with a high velocity (up to 200 km s−1). They are produced by dynamical ejections in young massive clusters or by supernova explosions in massive binaries. OB runaways can travel several hundred parsec before exploding as...

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Detalhes bibliográficos

Principais autores:	Azatyan N., Kaper L., Samsonyan A., Stoop M., Andreasyan D., van den Eijnden J., Nikoghosyan E.
Formato:	Artigo
Idioma:	Inglês
Publicado em:	EDP Sciences 2026-05-01
coleção:	Astronomy & Astrophysics
Assuntos:	binaries: general stars: early-type stars: mass-loss open clusters and associations: individual: velob1 x-rays: binaries
Acesso em linha:	https://www.aanda.org/articles/aa/full_html/2026/05/aa59021-26/aa59021-26.html
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