IDENTIFYING CONTRIBUTIONS TO THE STELLAR HALO FROM ACCRETED, KICKED-OUT, AND IN SITU POPULATIONS.

Autor: Sheffield, Allyson A.1 asheffield@astro.columbia.edu, Majewski, Steven R.2 srm4n@virginia.edu, Johnston, Kathryn V.1 kvj@astro.columbia.edu, Cunha, Katia3,4,5 cunha@noao.edu, Smith, Verne V.4 vsmith@noao.edu, Cheung, Andrew M.2,6 amc4e@virginia.edu, Hampton, Christina M.2, David, Trevor J.7 tjd@astro.caltech.edu, Wagner-Kaiser, Rachel8 rawagnerkaiser@astro.ufl.edu, Johnson, Marshall C.9 mjohnson@astro.as.utexas.edu, Kaplan, Evan10 evakaplan@vassar.edu, Miller, Jacob10, Patterson, Richard J.2 rjp0i@virginia.edu
Zdroj: Astrophysical Journal. 12/20/2012, Vol. 761 Issue 2, p1-1. 1p.
Databáze: Academic Search Ultimate