Spectroscopic evolution of very massive stars at z = 1/2.5 z⊙

HIGHLIGHTS

• who: Martins F. and Palacios A. from the Universitu00e9 de Montpellier, CNRS, Place Eugu00e8ne Bataillon, Montpellier, France have published the paper: Spectroscopic evolution of very massive stars at Z = 1/2.5 Zu2299, in the Journal: (JOURNAL)
• what: The authors show that the optical and UV range is dominated by He II 4686 and He II 1640 emission for almost the entire mainsequence evolution of VMSs in contrast to less massive stars. The authors show that stars with masses higher than 100 M emit nearly as much light as all other stars in young starbursts . . .
  

   

  

  If you want to have access to all the content you need to log in!

  Thanks :)

  Username or E-mail:

  If you don't have an account, you can create one here.