The mass-loss return from evolved stars to the Large Magellanic Cloud-Reference-Cited by-同舟云学术

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The mass-loss return from evolved stars to the Large Magellanic Cloud

Published:2010-11-23 Issue: Volume:524 Page:A49
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Srinivasan S.,Sargent B. A.,Matsuura M.,Meixner M.,Kemper F.,Tielens A. G. G. M.,Volk K.,Speck A. K.,Woods P. M.,Gordon K.,Marengo M.,Sloan G. C.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201014991/pdf

Reference91 articles.

1. SpitzerSAGE Survey of the Large Magellanic Cloud. II. Evolved Stars and Infrared Color-Magnitude Diagrams

2. AGB stars in the Magellanic Clouds

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1. Searching for Anomalies in the ZTF Catalog of Periodic Variable Stars;The Astrophysical Journal;2022-06-01

2. The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope;Monthly Notices of the Royal Astronomical Society;2022-03-17

3. The role of dust destruction and dust growth in the evolution of the interstellar medium;Monthly Notices of the Royal Astronomical Society;2020-06-04

4. Characterization of M-stars in the LMC in the JWST era;Monthly Notices of the Royal Astronomical Society;2020-02-10

5. Evolved stars in the Local Group galaxies – III. AGB and RSG stars in Sextans A;Monthly Notices of the Royal Astronomical Society;2018-10-30

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