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IRAS 17393-3004, a late-type supergiant surrounded by a dust shell

Sabine Philipp·Richard J. Tuffs·Peter G. Mezger·Robert Zylka
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Abstract

Infrared observations of IRAS 17393-3004, including a full scan ISOSWS are presented. The ISOSWS spectrum shows two prominent dust emission peaks at lambda 10.4mu and 17.5mu confirming that the source is a luminous star surrounded by a dust shell. The spectrum of the star, deduced from modeling of the radiative transfer through a spherical shell using the DUSTY code (Ivezic et al. 1997), can be explained along with other known properties in terms of an M4 supergiant with OH, SiO and H_2O maser emission and a large mass loss of ~ 10^{-4}M(sun)yr^{-1}.

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Sabine Philipp, Richard J. Tuffs, Peter G. Mezger, Robert Zylka. 1999-08-24. IRAS 17393-3004, a late-type supergiant surrounded by a dust shell. https://arxiv.org/abs/astro-ph/9908264

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