SIMBAD references

1999A&A...344..918J - Astronomy and Astrophysics, volume 344, 918-922 (1999/4-3)

IRAS 03313+6058: an AGB star with 30 micron emission.


Abstract (from CDS):

This paper reports a detection of the 30 micron emission feature from the C-rich Asymptotic Giant Branch (AGB) star IRAS 03313+6058 based on the ISO-SWS observation. Modeling of the spectral energy distribution shows that this emission starts at about 20 micron and possibly extends to the limit (45 micron) of the observation. By assuming MgS as the carrier, the number ratio of Sulfur atoms in MgS to Hydrogen atoms in total, n(S)/n(H), is 3.0x10–6 as derived from model fitting. A comparison is made between this emission feature and other AGB and post-AGB objects.

Abstract Copyright:

Journal keyword(s): stars: individual: IRAS 03313+6058 - stars: circumstellar matter - stars: chemically peculiar - stars: AGB and post-AGB

Simbad objects: 10

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