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Discovery of water vapour in the carbon star V Cygni from observations with Herschel/HIFI

Neufeld, D. A. (author)
Johns Hopkins University
Gonzalez-Alfonso, E. (author)
Universidad de Alcala,University of Alcalá
Melnick, G. J. (author)
Harvard-Smithsonian Center for Astrophysics
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Pulecka, M. (author)
Polish Academy of Sciences,European Space Astronomy Centre (ESAC)
Schmidt, M. (author)
Polish Academy of Sciences
Szczerba, R. (author)
Polish Academy of Sciences
Bujarrabal, V. (author)
Alcolea, J. (author)
Cernicharo, J. (author)
Centro de Astrobiologia (CAB)
Decin, L. (author)
Universiteit Van Amsterdam,University of Amsterdam,Katholieke Universiteit Leuven
Dominik, C. (author)
Universiteit Van Amsterdam,University of Amsterdam,Radboud Universiteit,Radboud University
Justtanont, Kay, 1965 (author)
Chalmers tekniska högskola,Chalmers University of Technology
de Koter, A. (author)
Universiteit Van Amsterdam,University of Amsterdam
Marston, A. P. (author)
European Space Astronomy Centre (ESAC),Atacama Large Millimeter-submillimeter Array (ALMA)
Menten, K. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Olofsson, Hans, 1952 (author)
Stockholms universitet,Institutionen för astronomi,Chalmers tekniska högskola,Chalmers University of Technology
Planesas, P. (author)
Atacama Large Millimeter-submillimeter Array (ALMA)
Schöier, Fredrik, 1969 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Teyssier, D. (author)
European Space Astronomy Centre (ESAC),Atacama Large Millimeter-submillimeter Array (ALMA)
Waters, Lbfm (author)
Universiteit Van Amsterdam,University of Amsterdam,Katholieke Universiteit Leuven
Edwards, K. (author)
University of Waterloo
McCoey, C. (author)
University of Waterloo
Shipman, R. (author)
Netherlands Institute for Space Research (SRON)
Jellema, W. (author)
Netherlands Institute for Space Research (SRON)
de Graauw, T. (author)
Atacama Large Millimeter-submillimeter Array (ALMA)
Ossenkopf, V. (author)
Universität zu Köln,University of Cologne
Schieder, R. (author)
Universität zu Köln,University of Cologne
Philipp, S. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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 (creator_code:org_t)
2010-10-01
2010
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 521:1, s. Article Number: L5-
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We report the discovery of water vapour toward the carbon star V Cygni. We have used Herschel's HIFI instrument, in dual beam switch mode, to observe the 1(11)-0(00) para-water transition at 1113.3430 GHz in the upper sideband of the Band 4b receiver. The observed spectral line profile is nearly parabolic, but with a slight asymmetry associated with blueshifted absorption, and the integrated antenna temperature is 1.69 +/- 0.17 K km s(-1). This detection of thermal water vapour emission, carried out as part of a small survey of water in carbon-rich stars, is only the second such detection toward a carbon-rich AGB star, the first having been obtained by the Submillimeter Wave Astronomy Satellite toward IRC+ 10216. For an assumed ortho-to-para ratio of 3 for water, the observed line intensity implies a water outflow rate similar to 3-6 x 10(-5) Earth masses per year and a water abundance relative to H-2 of similar to 2-5 x 10(-6). This value is a factor of at least 10(4) larger than the expected photospheric abundance in a carbon-rich environment, and - as in IRC+ 10216 - raises the intriguing possibility that the observed water is produced by the vapourisation of orbiting comets or dwarf planets. However, observations of the single line observed to date do not permit us to place strong constraints upon the spatial distribution or origin of the observed water, but future observations of additional transitions will allow us to determine the inner radius of the H2O-emitting zone, and the H2O ortho-to-para ratio, and thereby to place important constraints upon the origin of the observed water emission.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

giant branch stars
chemistry
submillimeter: stars
submillimeter
irc+10216
emission
circumstellar matter
circumstellar envelopes
stars: AGB and post-AGB
Astronomy and astrophysics

Publication and Content Type

art (subject category)
ref (subject category)

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