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An Ordered Envelope-Disk Transition in the Massive Protostellar Source G339.88-1.26

Zhang, Yichen (author)
RIKEN
Tan, Jonathan, 1973 (author)
University of Virginia,Chalmers tekniska högskola,Chalmers University of Technology
Sakai, N. (author)
RIKEN
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Tanaka, Kei E.I. (author)
Osaka University,National Astronomical Observatory of Japan
De Buizer, James M. (author)
NASA Ames Research Center
Liu, Mengyao (author)
University of Virginia
Beltrán, M. T. (author)
Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory
Kratter, K. M. (author)
University of Arizona
Mardones, Diego (author)
Universidad de Chile (UCH),University of Chile (UCH)
Garay, G. (author)
Universidad de Chile (UCH),University of Chile (UCH)
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 (creator_code:org_t)
2019-03-06
2019
English.
In: Astrophysical Journal. - : American Astronomical Society. - 1538-4357 .- 0004-637X. ; 873:1
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We report molecular line observations of the massive protostellar source G339.88-1.26 with the Atacama Large Millimeter/Submillimeter Array. The observations reveal a highly collimated SiO jet extending from the 1.3 mm continuum source, which connects to a slightly wider but still highly collimated CO outflow. Rotational features perpendicular to the outflow axis are detected in various molecular emissions, including SiO, SO 2 , H 2 S, CH 3 OH, and H 2 CO emissions. Based on their spatial distributions and kinematics, we find that they trace different parts of the envelope-disk system. The SiO emission traces the disk and inner envelope in addition to the jet. The CH 3 OH and H 2 CO emissions mostly trace the infalling-rotating envelope and are enhanced around the transition region between envelope and disk, i.e., the centrifugal barrier. The SO 2 and H 2 S emissions are enhanced around the centrifugal barrier and also trace the outer part of the disk. Envelope kinematics are consistent with rotating-infalling motion, while those of the disk are consistent with Keplerian rotation. The radius and velocity of the centrifugal barrier are estimated to be about 530 au and 6 , respectively, leading to a central mass of about 11 M o , consistent with estimates based on spectral energy distribution fitting. These results indicate that an ordered transition from an infalling-rotating envelope to a Keplerian disk through a centrifugal barrier, accompanied by changes of types of molecular line emissions, is a valid description of this massive protostellar source. This implies that at least some massive stars form in a similar way to low-mass stars via core accretion.

Subject headings

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)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Keyword

stars: massive
stars: formation
ISM: individual objects (G339.88-1.26)
ISM: jets and outflows
ISM: molecules
ISM: kinematics and dynamics

Publication and Content Type

art (subject category)
ref (subject category)

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