Phylogeny of the milky way’s inner disk and bulge populations: implications for gas accretion, (the lack of) inside-out thick disk formation, and quenching

HIGHLIGHTS

• who: Haywood Misha and colleagues from the GEPI, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Paris Cité, place Jules Janssen, Meudon, France have published the article: Phylogeny of the Milky Way’s inner disk and bulge populations: Implications for gas accretion, (the lack of) inside-out thick disk formation, and quenching, in the Journal: (JOURNAL)
• what: The authors show that the and the of the Milky Way (MW) at R. The authors show that at z ≤ 1.5 when the MW was starting to quench transitioning between the end of the α-enhanced thick formation . . .
  

   

  

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

  Thanks :)

  Username or Email

  Password

  Remember me

  Lost your password?

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