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  • Origin High-mass X-ray binary

Highlights

Origin of the high-mass X-ray binary 4U 2206+54/BD +53 2790
in a supernova 2.8 Myr ago

1914x828 

Traceback motion of high-mass X-ray binary 4U 2206+54/BD +53 2790 and BD+23 2820 to the Cep OB1 association,
where a supernova in a binary star happened 2.8 million years ago.
  Paper by Hambaryan et al. MNRAS 2022, in press  
 
  Previous features  

Erstellt: J. Weiprecht, 04.02.2022, Mod. 08.02.2022 JW

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