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Mid and far-infrared spectra of the third brightest carbon star IRAS 15194-5115
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory. Physics, Department of Astronomy and Space Physics.
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1998 (English)In: Asymptotic Giant Branch Stars, IAU Symposium 191, 1998Conference paper (Other scientific)
Abstract [en]

ISO observations from 2 to 197 microns of the recently discovered, third brightest (at 12 microns) carbon star IRAS 15194-5115, are analysed.

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Keyword [en]
infrared : stars; stars : late-type; stars : circumstellar matter; stars : AGB and post-AGB; ENVELOPES
URN: urn:nbn:se:uu:diva-34852OAI: oai:DiVA.org:uu-34852DiVA: diva2:62751
Addresses: Ryde Nils, Univ Uppsala, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Univ Uppsala, Astron Observ, S-75120 Uppsala, Sweden.Available from: 2005-05-03 Created: 2005-05-03

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Ryde, NilsEriksson, KjellGustafsson, Bengt
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Astronomical observatoryDepartment of Astronomy and Space Physics

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