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arXiv:astro-ph/0009440 (astro-ph)
[Submitted on 27 Sep 2000]

Title:Water and Dust Emission from W Hydrae

Authors:Victor Zubko, Moshe Elitzur
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Abstract: We construct a self-consistent model for the wind around W Hya by solving the coupled equations describing the hydrodynamics and dust radiative transfer problems. The model matches simultaneously the observed continuum radiation and wind velocity profile. The water line emission is calculated next using the water abundance as the only free parameter, fitted from the ISO observations of Neufeld et al. (1996) and Barlow et al. (1996). The gas temperature is determined from a thermal balance calculation that includes water as one of its main components. Our model successfully fits all the observed water lines, resolving a major discrepancy between the modeling results of the two observing teams. The mass loss rate is 2.3 x 10^{-6} M_solar yr^{-1}, the water abundance is 1.0 x 10^{-4} and the ortho:para ratio is 1:1.3.
Comments: 5 pages, 3 figures, uses this http URL and this http URL, accepted by ApJ Letters
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/0009440
  (or arXiv:astro-ph/0009440v1 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/0009440
Related DOI: https://doi.org/10.1086/317317

Submission history

From: Viktor Zubko [view email]
[v1] Wed, 27 Sep 2000 14:50:26 UTC (47 KB)
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