Dusty circumstellar disks

Dusty circumstellar disks in orbit around main-sequence stars were discovered in 1983 by the infrared astronomical satellite. It was the first time material that was not another star had been seen in orbit around a main-sequence star other than our Sun. Since that time, analyses of data from the inf...

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Bibliographic Details
Main Author: Zuckerman, B
Format: Electronic Article
Language:English
Subjects:
Online Access:Texto completo

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245 1 0 |a Dusty circumstellar disks  |h [recurso electrónico] /  |c B. Zuckerman. 
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520 |a Dusty circumstellar disks in orbit around main-sequence stars were discovered in 1983 by the infrared astronomical satellite. It was the first time material that was not another star had been seen in orbit around a main-sequence star other than our Sun. Since that time, analyses of data from the infrared astronomical satellite, the infrared space observatory, and ground-based telescopes have enabled astronomers to paint a picture of dusty disks around numerous main-sequence and post-main-sequence stars. This review describes, primarily in an evolutionary framework, the properties of some dusty disks orbiting, first, pre–main-sequence stars, then main-sequence and post-main-sequence stars, and ending with white dwarfs. 
650 4 |a Stellar evolution 
650 4 |a White dwarfs 
650 4 |a Pre-main sequence 
650 4 |a Red giants 
773 |g vol. 39 2001  |t Annual Review of Astronomy and Astrophysics 
856 |u https://www.annualreviews.org/content/journals/10.1146/annurev.astro.39.1.549  |y Texto completo 
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