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The nature of the circumstellar CO2 emission from M giants
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory. Physics, Department of Astronomy and Space Physics.
1999 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 341, no 2, 579-586 p.Article in journal (Refereed) Published
Abstract [en]

The 13-16 mu m region observed by the Infrared Space Observatory (ISO) of several ABG stars are discussed. We present and analyse spectra of seven M giants which show carbon dioxide features. To explain the features of the bands, we suggest they originate

Place, publisher, year, edition, pages
1999. Vol. 341, no 2, 579-586 p.
Keyword [en]
infrared : stars; stars : late-type; stars : circumstellar matter; stars : AGB and post-AGB; ENVELOPES
Identifiers
URN: urn:nbn:se:uu:diva-85284OAI: oai:DiVA.org:uu-85284DiVA: diva2:113192
Note
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 Last updated: 2011-01-14

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Ryde, NilsEriksson, KjellGustafsson, Bengt

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