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Growth of planetesimals and clearance of disks around the T-tauri stars

โœ Scribed by K. M. Guseinov


Publisher
Springer Netherlands
Year
1988
Tongue
English
Weight
347 KB
Volume
43
Category
Article
ISSN
1573-0794

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We have used the James Clerk Maxwell Telescope in Hawaii to search at submillimeter wavelengths for continuum emission from dust, and spectral line emission from carbon monoxide (CO) gas, in the neighborhood of HR 4796A. This young star has a dusty disk with a central cavity, where planets may have