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Sökning: id:"swepub:oai:research.chalmers.se:288825ea-fbb2-46c1-9889-94fc2905e309" > First Images of the...

First Images of the Molecular Gas around a Born-again Star Revealed by ALMA

Tafoya, Daniel, 1981 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Toala, Jesus A. (författare)
Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico
Unnikrishnan, Ramlal, 1997 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
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Vlemmings, Wouter, 1974 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Guerrero, Martin A. (författare)
Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)
Kimeswenger, Stefan (författare)
University of Innsbruck,Universidad Catolica del Norte
van Hoof, Peter A. M. (författare)
Royal Observatory of Belgium
Zapata, Luis A. (författare)
Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico
Treviño Morales, Sandra, 1985 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Rodriguez-Gonzalez, Janis B. (författare)
Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico
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 (creator_code:org_t)
2022-01-24
2022
Engelska.
Ingår i: Astrophysical Journal Letters. - : American Astronomical Society. - 2041-8213 .- 2041-8205. ; 925:1
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
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  • Born-again stars allow probing stellar evolution in human timescales and provide the most promising path for the formation of hydrogen-deficient post-asymptotic giant branch objects, but their cold and molecular components remain poorly explored. Here we present ALMA observations of V 605 Aql that unveil for the first time the spatio-kinematic distribution of the molecular material associated with a born-again star. Both the continuum and molecular line emission exhibit a clumpy ring-like structure with a total extent of approximate to 1 '' in diameter. The bulk of the molecular emission is interpreted as being produced in a radially expanding disk-like structure with an expansion velocity v(exp) similar to 90 km s(-1) and an inclination i approximate to 60 degrees with respect to the line of sight. The observations also reveal a compact high-velocity component, v(exp) similar to 280 km s(-1), that is aligned perpendicularly to the expanding disk. This component is interpreted as a bipolar outflow with a kinematical age tau less than or similar to 20 yr, which could either be material that is currently being ejected from V 605 Aql, or is being dragged from the inner parts of the disk by a stellar wind. The dust mass of the disk is in the range M-dust similar to 0.2-8 x 10(-3) M-circle dot, depending on the dust absorption coefficient. The mass of the CO is MCO approximate to 1.1 x 10(-5) M-circle dot, which is more than three orders of magnitude larger than the mass of the other detected molecules. We estimate a C-12/C-13 ratio of 5.6 +/- 0.6, which is consistent with the single stellar evolution scenario in which the star experienced a very late thermal pulse instead of a nova-like event as previously suggested.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Den kondenserade materiens fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Condensed Matter Physics (hsv//eng)

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