Detection of infall in the protostar B335 with ALMA

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DOIResolve DOI: http://doi.org/10.1088/0004-637X/814/1/22
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TypeArticle
Journal titleThe Astrophysical Journal
ISSN0004-637X
Volume814
Issue1
Article number22
AbstractObservations of the isolated globule B335 with ALMA have yielded absorption features against the continuum that are redshifted from the systemic velocity in both HCN and HCO+ lines. These features provide unambiguous evidence for infall toward a central luminosity source. Previously developed models of inside-out collapse can match the observed line profiles of HCN and HCO+ averaged over the central 50 AU. At the new distance of 100 pc, the inferred infall radius is 0.012 pc, the mass infall rate is 3 × 10-6 Mo yr-1, the age is 5 × 104 years, and the accumulated mass in the central zone is 0.15 , most of which must be in the star or in parts of a disk that are opaque at 0.8 mm. The continuum detection indicates an optically thin mass (gas and dust) of only 7.5 × 10-4 in the central region, consistent with only a very small disk mass.
Publication date
PublisherIOP Publishing
LanguageEnglish
AffiliationNational Research Council Canada (NRC-CNRC); National Science Infrastructure
Peer reviewedYes
NPARC number21277405
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Record identifier5aea7357-3fad-44c4-93dd-1c86c1060a7b
Record created2016-03-09
Record modified2016-07-18
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