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[Untitled]

Authors :
Roc M. Cutri
Carl J. Rice
Ray W. Russell
S. M. Mazuk
Catherine C. Venturini
Michael L. Sitko
David K. Lynch
Richard J. Rudy
Richard C. Puetter
Source :
Astrophysics and Space Science. 279:57-64
Publication Year :
2002
Publisher :
Springer Science and Business Media LLC, 2002.

Abstract

IR spectroscopy and photometry in the 0.8–2.4 and 3–14 μmregions are reported for seven dates between March 21 1998 and July20 2000 UT. The shorter wavelength region displays a smooth continuum increasing to longerwavelengths that is indicative of the Wien tail of a Planck function. Only theHe I 1.0830 line is present early and it shows a P-Cygni profile which laterdisappears. The long wave spectra show a smooth continuum between 3 and 13μm that was well fit by a gray body at 1000 K. A weak, unidentifiedemission feature appears between 8 and 10 μm.

Details

ISSN :
0004640X
Volume :
279
Database :
OpenAIRE
Journal :
Astrophysics and Space Science
Accession number :
edsair.doi...........5d6883a5ae4b3b9b3424395609de6bbe
Full Text :
https://doi.org/10.1023/a:1014643906270