MUSTANG 3.3mm Observations of Low-mass Cores

Details MUSTANG 3.3mm Observations of Low-mass Cores MUSTANG 3.3mm Observations of Low-mass Cores

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21541424s&link_type=abstract

American Astronomical Society, AAS Meeting #215, #414.24; Bulletin of the American Astronomical Society, Vol. 42, p.258

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present observations of low-mass star-forming cores (L1527, L1448C, B335, L483) observed during 2009 with MUSTANG, the 3.3mm bolometer camera on the 100-m Green Bank Telescope. The 3.3mm emission may be used to constrain the fraction of emission coming from the envelope and disk. We present our initial model comparisons to observations of the dust emission surrounding the protostars. Comparison is made to interferometric observations of L1527. These observations demonstrate the feasibility of active surface observations with aperture efficiencies above 20% at 3mm with the GBT.

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