uu.seUppsala University Publications
Change search
ReferencesLink to record
Permanent link

Direct link
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
URN: urn:nbn:se:uu:diva-85284OAI: oai:DiVA.org:uu-85284DiVA: diva2:113192
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

Open Access in DiVA

No full text

Search in DiVA

By author/editor
Ryde, NilsEriksson, KjellGustafsson, Bengt
By organisation
Astronomical observatoryDepartment of Astronomy and Space Physics

Search outside of DiVA

GoogleGoogle Scholar
The number of downloads is the sum of all downloads of full texts. It may include eg previous versions that are now no longer available

Total: 190 hits
ReferencesLink to record
Permanent link

Direct link