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Modelling of molecular bands of oxygen-rich AGB stars
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, Published paper (Other scientific)
Abstract [en]

ISO observations of infrared molecular bands of oxygen-rich AGB stars are compared with synthetic spectra generated using model atmospheres

Place, publisher, year, edition, pages
1998.
Keywords [en]
circumstellar matter; infrared : stars; stars : late-type; stars : AGB and post-AGB; E stars : mass loss; LONG-WAVELENGTH SPECTROMETER; MOLECULAR ENVELOPE; EVOLVED STARS; CIRCUMSTELLAR ENVELOPES; O-CETI; DUST; ATMOSPHERE; VARIABLES
Identifiers
URN: urn:nbn:se:uu:diva-34856OAI: oai:DiVA.org:uu-34856DiVA, id: diva2:62755
Note
Addresses: Ryde Nils, Univ Uppsala, Astron Observ, S-75120 Uppsala, Sweden. Univ Uppsala, Astron Observ, S-75120 Uppsala, Sweden. Onsala Space Observ, S-43992 Onsala, Sweden. Stockholm Observ, S-13336 Saltsjobaden, Sweden.Available from: 2005-05-03 Created: 2005-05-03

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Ryde, NilsEriksson, KjellGustafsson, Bengt

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