Observations of Dusty Disks

Details Observations of Dusty Disks Observations of Dusty Disks

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..713...83w&link_type=abstract

THE SEARCH FOR OTHER WORLDS: Fourteenth Astrophysics Conference. AIP Conference Proceedings, Volume 713, pp. 83-92 (2004).

Astronomy and Astrophysics

Astrophysics

1

Infrared Excess, Debris Disks, Protoplanetary Disks, Exo-Zodiacal Dust, Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers

Scientific paper

Dusty disks, those that have largely lost their gas as their host stars evolve onto the zero age main sequence, are interesting because of what they tell us about the conditions for planet formation. In the time period of 5-30 Myr, in our own Solar System, the gas giants may still have been forming and terrestrial planets were almost certainly still forming. This proceeding reviews the imaging and spectroscopy of young debris disks in stages analogous to the early Solar System.

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