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The carbon star IRAS 15194-5115: circumstellar CO radio and FIR rotational lines
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. 345, no 3, 841-846 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
1999. Vol. 345, no 3, 841-846 p.
Keyword [en]
stars : AGB and post-AGB; stars : circumstellar matter; stars : individual : IRAS15194-5115; stars : late-type; infrared : stars; LONG-WAVELENGTH SPECTROMETER; DUST SHELLS; ENVELOPES; IRAS-15194-5115; COEFFICIENTS; IRC+10216; OXYGEN
URN: urn:nbn:se:uu:diva-85278OAI: oai:DiVA.org:uu-85278DiVA: diva2:113186
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: 2011-01-14

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