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Resolved CO 4.6 um Line Emission from Inner Circumstellar Envelopes -- the Case of Mira
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory. Physics, Department of Astronomy and Space Physics.
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1999 (English)In: 2nd Austrian ISO Workshop, 1999, 66- p.Conference paper (Other scientific)
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. 66- p.
Keyword [en]
infrared : stars; stars : late-type; stars : circumstellar matter; stars : AGB and post-AGB; ENVELOPES
URN: urn:nbn:se:uu:diva-34862OAI: oai:DiVA.org:uu-34862DiVA: diva2:62761
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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