MAPPING THE STELLAR STRUCTURE OF THE MILKY WAY THICK DISK AND HALO USING SEGUE PHOTOMETRY-Reference-Cited by-同舟云学术

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MAPPING THE STELLAR STRUCTURE OF THE MILKY WAY THICK DISK AND HALO USING SEGUE PHOTOMETRY

Published:2010-04-13 Issue:1 Volume:714 Page:663-674
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

de Jong Jelte T. A.,Yanny Brian,Rix Hans-Walter,Dolphin Andrew E.,Martin Nicolas F.,Beers Timothy C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/714/i=1/a=663/pdf

Reference59 articles.

1. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY

2. The universe at faint magnitudes. I - Models for the galaxy and the predicted star counts

3. The Accretion Origin of the Milky Way’s Stellar Halo

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