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

Direct link
Modeling CO emission from Mira's wind
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Faculty of Science and Technology, Astronomical observatory.
2001 (English)In: ASTROPHYSICAL JOURNAL, ISSN 0004-637X, Vol. 547, no 1, 384-392 p.Article in journal (Refereed) Published
Abstract [en]

We have modeled the circumstellar envelope of o Ceti (Mira) using new observational constraints. These are obtained from photospheric light scattered in near-IR vibrational-rotational lines of circumstellar CO molecules at 4.6 mum: absolute fluxes, the ra

Place, publisher, year, edition, pages
2001. Vol. 547, no 1, 384-392 p.
Keyword [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
URN: urn:nbn:se:uu:diva-36662OAI: oai:DiVA.org:uu-36662DiVA: diva2:64561
Addresses: Ryde N, Uppsala Astron Observ, Box 515, SE-75120 Uppsala, Sweden. Uppsala Astron Observ, SE-75120 Uppsala, Sweden. Stockholm Observ, SE-13336 Saltsjobaden, Sweden.Available from: 2005-05-03 Created: 2005-05-03 Last updated: 2011-01-13

Open Access in DiVA

No full text

Search in DiVA

By author/editor
Ryde, Nils
By organisation
Department of Astronomy and Space PhysicsAstronomical observatory

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: 179 hits
ReferencesLink to record
Permanent link

Direct link