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Probing the mass loss history of carbon stars using CO line and dust continuum emission
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory.
2002 (English)In: Astronomy and Astrophysics, Vol. 391, 577- p.Article in journal (Refereed) Published
Abstract [en]

We have modelled radio and far-infrared rotational lines of (CO)-C-12 and (CO)-C-13 Obtained from the circumstellar envelope of the infrared-bright carbon star IRAS 15194-5115. Eleven rotational lines between J=1-0 and 21-20 and nine rotational lines betw

Place, publisher, year, edition, pages
2002. Vol. 391, 577- p.
Identifiers
URN: urn:nbn:se:uu:diva-48066OAI: oai:DiVA.org:uu-48066DiVA: diva2:75973
Note
Addresses: Ryde Nils, Univ Uppsala, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Univ Uppsala, Astron Observ, S-75120 Uppsala, Sweden. Stockholm Observ, S-13336 Saltsjobaden, Sweden.Available from: 2005-05-03 Created: 2005-05-03 Last updated: 2011-01-13

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