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Observations of dust emission from vega-excess stars

โœ Scribed by R. J. Sylvester; M. J. Barlow; C. J. Skinner

Publisher
Springer Netherlands
Year
1995
Tongue
English
Weight
186 KB
Volume
224
Category
Article
ISSN
0004-640X

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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 ยตm) has been used to map the area around the stars to establish