Dusty debris clouds around main sequence and post-main sequence stars

Details Dusty debris clouds around main sequence and post-main sequence stars Dusty debris clouds around main sequence and post-main sequence stars

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...36..303z&link_type=abstract

In: Planets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992 (A93-36

Physics

13

Cosmic Dust, Late Stars, Main Sequence Stars, Planetary Systems, Stellar Envelopes, Stellar Evolution, White Dwarf Stars

Scientific paper

During the past decade, infrared observations by IRAS and from the ground have revealed that many stars are orbited by dusty debris disks. Somewhat more indirect arguments indicate that many of these systems also contain asteroids, comets, and/or planets, thereby suggesting that planetary systems may be quite common in the Milky Way. Dust clouds at the main sequence K5 star HD 98800 and the white dwarf Giclas 29-38 are particularly noteworthy and mysterious.

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