ISO observations of far-infrared rotational emission lines of water vapor toward the supergiant star VY Canis Majoris

Details ISO observations of far-infrared rotational emission lines of water vapor toward the supergiant star VY Canis Majoris ISO observations of far-infrared rotational emission lines of water vapor toward the supergiant star VY Canis Majoris

1999-03-31

arxiv.org/abs/astro-ph/9903480v1

Astronomy and Astrophysics

Astrophysics

11 pages (inc. 2 figures), LaTeX, uses aaspp4.sty, accepted for publication in ApJ Letters

Scientific paper

10.1086/312036

We report the detection of numerous far-infrared emission lines of water vapor toward the supergiant star VY Canis Majoris. A 29.5 - 45 micron grating scan of VY CMa, obtained using the Short Wavelength Spectrometer (SWS) of the Infrared Space Observatory (ISO) at a spectral resolving power of approximately 2000, reveals at least 41 spectral features due to water vapor that together radiate a total luminosity ~ 25 solar luminosities. In addition to pure rotational transitions within the ground vibrational state, these features include rotational transitions within the (010) excited vibrational state. The spectrum also shows the doublet Pi 1/2 (J=5/2) <-- doublet Pi 3/2 (J=3/2) OH feature near 34.6 micron in absorption. Additional SWS observations of VY CMa were carried out in the instrument's Fabry-Perot mode for three water transitions: the 7(25)-6(16) line at 29.8367 micron, the 4(41)-3(12) line 31.7721 micron, and the 4(32)-3(03) line at 40.6909 micron. The higher spectral resolving power of approximately 30,000 thereby obtained permits the line profiles to be resolved spectrally for the first time and reveals the "P Cygni" profiles that are characteristic of emission from an outflowing envelope.

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