Terrestrial-temperature dust around main sequence stars

Details Terrestrial-temperature dust around main sequence stars Terrestrial-temperature dust around main sequence stars

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998exdu.work..107b&link_type=abstract

Exozodiacal Dust Workshop, p. 107

Astronomy and Astrophysics

Astronomy

4

Main Sequence Stars, Planetary Evolution, Interstellar Matter, Space Debris, Dust, Infrared Astronomy Satellite, Terrestrial Planets, Stellar Evolution

Scientific paper

This paper will briefly review the main sequence debris disks discovered by IRAS, including the beta Pic system which is a well-studied example containing some dust at terrestrial planet temperatures. A few more systems with warm dust will then be considered, followed by a brief discussion of the evolutionary status of these systems and their connection to planet formation.

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