Searching for a kinematic signature of the moderately metal-poor stars in the milky way bulge using n-body simulations

HIGHLIGHTS

• who: Gómez A. et al. from the Université PSL, CNRS, Place Jules Janssen, Meudon, France have published the Article: Searching for a kinematic signature of the moderately metal-poor stars in the Milky Way bulge using N-body simulations, in the Journal: (JOURNAL)
• what: The authors compare the predicted results with ARGOS data and APOGEE DR13 data and show that moderately metal-poor stars are well reproduced with the co-spatial stellar discs model which has massive thick disc. The paper is organised as follows: in Sect 2, the models are briefly described.
 



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.