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MIRA's wind explored in scattering infrared CO lines
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory.
2000 (English)In: ASTROPHYSICAL JOURNAL, ISSN 0004-637X, Vol. 545, no 2, 945-956 p.Article in journal (Refereed) Published
Abstract [en]

We have observed the intermediate regions of the circumstellar envelope of Mira (o Ceti) in photospheric light scattered by three vibration-rotation transitions of the fundamental band of CO, from low-excited rotational levels of the ground vibrational st

Place, publisher, year, edition, pages
2000. Vol. 545, no 2, 945-956 p.
Keyword [en]
circumstellar matter; infrared : stars; stars : AGB and post-AGB; stars : individual (o Ceti); stars : late-type; stars : mass loss; MASS-LOSS RATES; GIANT BRANCH STARS; CIRCUMSTELLAR ENVELOPES; MOLECULAR ENVELOPE; ATMOSPHERIC STRUCTURE; MODEL ATMOSPHERES
URN: urn:nbn:se:uu:diva-36661OAI: oai:DiVA.org:uu-36661DiVA: diva2:64560
Addresses: Ryde N, Uppsala Astron Observ, Box 515, S-75120 Uppsala, Sweden. Uppsala Astron Observ, S-75120 Uppsala, Sweden. Natl Opt Astron Observ, Tucson, AZ 85726 USA.Available from: 2005-05-03 Created: 2005-05-03 Last updated: 2011-01-14

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Ryde, NilsGustafsson, BEriksson, K
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