THE ORIGIN OF THE SPLIT RED CLUMP IN THE GALACTIC BULGE OF THE MILKY WAY-Reference-Cited by-同舟云学术

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THE ORIGIN OF THE SPLIT RED CLUMP IN THE GALACTIC BULGE OF THE MILKY WAY

Published:2012-08-09 Issue:1 Volume:756 Page:22
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Ness M.,Freeman K.,Athanassoula E.,Wylie-De-Boer E.,Bland-Hawthorn J.,Lewis G. F.,Yong D.,Asplund M.,Lane R. R.,Kiss L. L.,Ibata R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/756/i=1/a=22/pdf

Reference29 articles.

1. K‐Band Calibration of the Red Clump Luminosity

2. What determines the strength and the slowdown rate of bars?

3. On the nature of bulges in general and of box/peanut bulges in particular: input fromN-body simulations

4. JHKLM photometry - Standard systems, passbands, and intrinsic colors

5. K-band observations of boxy bulges - I. Morphology and surface brightness profiles

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