HCO^+^ (J=4-3) mapping of the molecular disk around IRS 7 in Corona Australis.

Details HCO^+^ (J=4-3) mapping of the molecular disk around IRS 7 in Corona Australis. HCO^+^ (J=4-3) mapping of the molecular disk around IRS 7 in Corona Australis.

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...326..366a&link_type=abstract

Astronomy and Astrophysics, v.326, p.366-372

Astronomy and Astrophysics

Astrophysics

7

Stars: Formation, Stars: Individual: R Cra Irs 7, Ism: Jets And Outflows, Ism: Kinematics And Dynamics, Radio Lines: Ism

Scientific paper

Submillimetre HCO^+^(J=4-3) mapping observations of the immediate
environs of the infrared source IRS 7 in Corona Australis have provided
corroborative evidence for the existence of the rotating molecular disk
detailed in our earlier paper. An improved estimate of
0.8Msun_ for the mass of the central protostar is obtained.

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