Observations of Disks around Protostellar Sources with Nobeyama Millimeter Array

Details Observations of Disks around Protostellar Sources with Nobeyama Millimeter Array Observations of Disks around Protostellar Sources with Nobeyama Millimeter Array

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224...13o&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 13-16

Astronomy and Astrophysics

Astrophysics

1

Circumstellar Disks, Disk Formation, Dynamical Accretion, Hl Tau

Scientific paper

We present results from a survey observation of circumstellar disks around protostellar sources associated with the Taurus molecular cloud. Our result shows that the 98 GHz continuum emission tends to be weaker for embedded sources than for visible T Tauri stars, which is consistent with our previous interpretation of disk formation. Direct observations of the formation of a centrifugally supported viscous accretion disk around HL Tau is discussed.

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