Gas to dust ratios in Vega-excess stars

Details Gas to dust ratios in Vega-excess stars Gas to dust ratios in Vega-excess stars

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..393..209c&link_type=abstract

The seventh astrophysical conference: Star formation, near and far. AIP Conference Proceedings, Volume 393, pp. 209-213 (1997).

Astronomy and Astrophysics

Astrophysics

1

Pre-Main Sequence Objects, Young Stellar Objects And Protostars, Near Infrared, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

We report new infrared photometry of a sample of Vega-excess systems,
and the results of a search for submillimeter CO emission. The resulting
gas to dust ratios are compared with those for the class archetypes, and
are found to be similarly reduced from the canonical molecular cloud
value.

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