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Constraining the Infalling Envelope Models of Embedded Protostars: BHR 71 and Its Hot Corino

Yang, Yao-Lun (author)
The University of Texas at Austin, USA,RIKEN
Evans, (author)
The University of Texas at Austin, USA,Kyung Hee University,Korea Astronomy and Space Science Institute
Smith, Aaron (author)
Massachusetts Institute of Technology (MIT)
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Lee, Jeong-Eun (author)
Kyung Hee University
Tobin, John J. (author)
The University of Oklahoma,National Radio Astronomy Observatory
Terebey, Susan (author)
The California State University, United States
Calcutt, Hannah, 1988 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Jorgensen, Jes K. (author)
Köpenhamns universitet,University of Copenhagen
Green, Joel D. (author)
The University of Texas at Austin, USA,Space Telescope Science Institute (STScI)
Bourke, Tyler L. (author)
SKA Organisation
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 (creator_code:org_t)
2020-03-04
2020
English.
In: Astrophysical Journal. - : American Astronomical Society. - 1538-4357 .- 0004-637X. ; 891:1
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The collapse of a protostellar envelope results in the growth of a protostar and the development of a protoplanetary disk, playing a critical role during the early stages of star formation. Characterizing the gas infall in the envelope constrains the dynamical models of star formation. We present unambiguous signatures of infall, probed by optically thick molecular lines, toward an isolated embedded protostar, BHR 71 IRS1. The three-dimensional radiative transfer calculations indicate that a slowly rotating infalling envelope model following the "inside-out" collapse reproduces the observations of both lines, as well as the low-velocity emission of the HCN line. The envelope has a model-derived ag lines, where outflows or a Keplerian disk may contribute. The ALMA observations serendipitously discover the emission of complex organic molecules (COMs) concentrated within a radius of 100 au, indicating that BHR 71 IRS1 harbors a hot corino. Eight species of COMs are identified, including CH3OH and CH3OCHO, along with H2CS, SO2 and HCN v(2) = 1. The emission of methyl formate and C-13-methanol shows a clear velocity gradient within a radius of 50 au, hinting at an unresolved Keplerian rotating disk.

Subject headings

NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Meteorologi och atmosfärforskning (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Meteorology and Atmospheric Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)

Keyword

Star formation
Bok globules
Gravitational collapse
Radiative transfer
Astrochemistry
Protostars

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