Location and phase of dust formation in IRC + 10216 indicated by 11 micron spatial interferometry-Reference-Cited by-同舟云学术

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Location and phase of dust formation in IRC + 10216 indicated by 11 micron spatial interferometry

Published:1990-08 Issue: Volume:359 Page:L59
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Danchi W. C.,Bester M.,Degiacomi C. G.,McCullough P. R.,Townes C. H.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 50 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Detection of the S(1) Rotational Line of H₂ toward IRC+10216: A Simultaneous Measurement of the Mass-loss Rate and CO Abundance;The Astrophysical Journal Letters;2022-03-01

2. FORMATION OF SiC GRAINS IN PULSATION-ENHANCED DUST-DRIVEN WIND AROUND CARBON-RICH ASYMPTOTIC GIANT BRANCH STARS;The Astrophysical Journal;2012-01-16

3. FOUR DECADES OF IRC +10216: EVOLUTION OF A CARBON-RICH DUST SHELL RESOLVED AT 10 μm WITH MMT ADAPTIVE OPTICS AND MIRAC4,,;The Astrophysical Journal;2011-12-22

4. The mass-loss return from evolved stars to the Large Magellanic Cloud;Astronomy & Astrophysics;2010-11-23

5. A Review of AGB Mass Loss Imaging Techniques;Publications of the Astronomical Society of Australia;2009

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