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Models of dusty envelopes around Vega-like stars

✍ Scribed by A. B. Men'Shchikov

Publisher
John Wiley and Sons
Year
1989
Tongue
English
Weight
178 KB
Volume
310
Category
Article
ISSN
0004-6337

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The photometer (ISOPHOT) on the Infrared Space Observatory (ISO) has proved to be invaluable for investigating the dust around main sequence stars (both prototypes and candidate Vegalike stars). The long wavelength camera (at 60 and 90 Β΅m) has been used to map the area around the stars to establish