SIMBAD references

1999A&A...350..582P - Astronomy and Astrophysics, volume 350582-586 (1999/10-2)

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

PHILIPP S., TUFFS R.J., MEZGER P.G. and ZYLKA R.

Abstract (from CDS):

Infrared observations of IRAS17393-3004, including a full scan ISOSWS are presented. The ISOSWS spectrum shows two prominent dust emission peaks at λ 10.4µm and 17.5µm 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, User Manual for DUSTY, http://www.pa.uky.edu/~moshe/dusty), can be explained along with other known properties in terms of an M4 supergiant with OH, SiO and H2O maser emission and a large mass loss of ∼10–4M☉/yr.

Abstract Copyright: ∼

Journal keyword(s): stars: supergiants - stars: late-type - stars: fundamental parameters - stars: winds, outflows - infrared: stars

CDS comments: Table 1 : AFGL 1977 misprint for 1997

Simbad objects: 1

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