The dust debris around HR 4796

Details The dust debris around HR 4796 The dust debris around HR 4796

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...383l..79j&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 383, Dec. 20, 1991, p. L79, L80. Research supported by NASA.

Astronomy and Astrophysics

Astronomy

37

A Stars, Cosmic Dust, Main Sequence Stars, Stellar Envelopes, Infrared Astronomy Satellite, Optical Thickness

Scientific paper

The IRAS data strongly suggest that there is dust debris around the
main-sequence A star HR 4796. The optical depth of the dust cloud around
HR 4796 is probably twice that around Beta Pic, the main-sequence star
in the Bright Star Catalog which was previously thought to have the most
opaque dust debris cloud.

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