Astronomy and Astrophysics – Astronomy
Scientific paper
May 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21642210e&link_type=abstract
American Astronomical Society, AAS Meeting #216, #422.10
Astronomy and Astrophysics
Astronomy
Scientific paper
We present an excellent candidate for observational verification of the first hydrostatic core (FHSC). The FHSC is a theoretically predicted phase in the low-mass star formation process (Larson 1969), between the initiation of core collapse the the formation of a true protostar; this large (5 AU), cool (100 K) hydrostatically supported core of molecular hydrogen has so far not been directly observed. We obtained deep Spitzer 70 micron images of a sample of seven target dense starless cores, and detected one, Per-Bolo 58, at the level expected for the FHSC. A low signal-to-noise detection at 24 micron leaves open the possibility that this could be a very low luminosity protostar, however. We use radiative transfer models (Dullemond & Dominik 2004) to determine the best-fitting FHSC and protostar to the spectral energy distribution (SED) and 2.9 mm intensity profile (Schnee et al. 2010) of Per-Bolo 58. The SED is consistent with a FHSC with some source of lower envelope opacity that allows 24 micron emission to escape: a small outflow cavity, a cavity in the envelope, or a clumpy envelope. Although we are unable to rule out the presence of a protostar, if present it would be one of the lowest luminosity protostars known (internal luminosity 0.01 Lsun).
Dunham Michael M.
Enoch Melissa
Harvey Paul
Lee Julian
Schnee Scott
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