CO depletion in the protoplanetary disk of β Pictoris

Details CO depletion in the protoplanetary disk of β Pictoris CO depletion in the protoplanetary disk of β Pictoris

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...285..467s&link_type=abstract

Astronomy and Astrophysics 285, 467-468 (1994)

Astronomy and Astrophysics

Astrophysics

9

Radio Lines: Stars, Stars: Circumstellar Matter, Stars: Individual, {Beta} Pic

Scientific paper

We present the first ^12^CO (J=1-0) observations of β Pictoris, the only star for which a protoplanetary disk has been observed in optical wavelengths also. The star and its circumstellar region does not present evidence of emission, down to T_rms_ = 10 mK. Our result confirms a similar ^12^CO deficiency found in previous studies on other stars with IR excess and with presumed protoplanetary disks or rings.

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