THE MASS-LOSS RETURN FROM EVOLVED STARS TO THE LARGE MAGELLANIC CLOUD. II. DUST PROPERTIES FOR OXYGEN-RICH ASYMPTOTIC GIANT BRANCH STARS-Reference-Cited by-同舟云学术

THE MASS-LOSS RETURN FROM EVOLVED STARS TO THE LARGE MAGELLANIC CLOUD. II. DUST PROPERTIES FOR OXYGEN-RICH ASYMPTOTIC GIANT BRANCH STARS

Published:2010-05-21 Issue:1 Volume:716 Page:878-890
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Sargent Benjamin A.,Srinivasan S.,Meixner M.,Kemper F.,Tielens A. G. G. M.,Speck A. K.,Matsuura M.,Bernard J.-Ph.,Hony S.,Gordon Karl D.,Indebetouw R.,Marengo M.,Sloan G. C.,Woods Paul M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/716/i=1/a=878/pdf

Reference111 articles.

1. Spherically Symmetric Model Atmospheres for Low‐Mass Pre–Main‐Sequence Stars with Effective Temperatures between 2000 and 6800 K

2. Distribution of dust about Omicron Ceti and Alpha Orionis based on 11 micron spatial interferometry

3. ISO mid-infrared spectroscopy of Galactic Bulge AGB stars

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