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The widespread occurence of water vapor in the circumstellar envelopes of carbon-rich AGB stars: first results from a survey with Herschel/HIFI | D. A. Neufeld
; E. González-Alfonso
; G. Melnick
; R. Szczerba
; M. Schmidt
; L. Decin
; J. Alcolea
; A. de Koter
; F. L. Schöier
; V. Bujarrabal
; J. Cernicharo
; C. Dominik
; K. Justtanont
; A. P. Marston
; K. Menten
; H. Olofsson
; P. Planesas
; D. Teyssier
; L. B. F. M. Waters
; | Date: |
15 Dec 2010 | Abstract: | We report the preliminary results of a survey for water vapor in a sample of
eight C stars with large mid-IR continuum fluxes: V384 Per, CIT 6, V Hya, Y
CVn, IRAS 15194-5115, V Cyg, S Cep, and IRC+40540. This survey, performed using
the HIFI instrument on board the Herschel Space Observatory, entailed
observations of the lowest transitions of both ortho- and para-water: the
556.936 GHz 1(10)-1(01) and 1113.343 GHz 1(11)-0(00) transitions, respectively.
Water vapor was unequivocally detected in all eight of the target stars. Prior
to this survey, IRC+10216 was the only carbon-rich AGB star from which thermal
water emissions had been discovered, in that case with the use of the
Submillimeter Wave Astronomy Satellite (SWAS). Our results indicate that
IRC+10216 is not unusual, except insofar as its proximity to Earth leads to a
large line flux that was detectable with SWAS. The water spectral line widths
are typically similar to those of CO rotational lines, arguing against the
vaporization of a Kuiper belt analog (Ford & Neufeld 2001) being the general
explanation for water vapor in carbon-rich AGB stars. There is no apparent
correlation between the ratio of the integrated water line fluxes to the 6.3
micron continuum flux - a ratio which measures the water outflow rate - and the
total mass-loss rate for the stars in our sample. | Source: | arXiv, 1012.3456 | Services: | Forum | Review | PDF | Favorites |
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