 |
|
|
|||||||||
The results of the spectroscopic monitoring with resolution 15000 up to 70000 of the hypergiants HD 168607 B9.5 Ia-0 and HD 168625 B5.5 Ia-0 confirm the membership of the both stars in the association Ser OB1, prove their spacial proximity and increase the probability that the stars are a physical pair.
|