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Stellar far-IR fluxes: How accurate are model predictions?
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1996 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 309, no 3, 849-860 p.Article in journal (Refereed) Published
Abstract [en]

We present the results of an analysis of the accuracy of predicted far infrared (FIR) fluxes of stars. Sources of errors are a) the input parameters for the model atmospheres; b) assumptions in the modelling, resulting in errors in the structure of the mo

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1996. Vol. 309, no 3, 849-860 p.
Keyword [en]
stars; atmospheres; infrared; stars; stars; fundamental parameters; INFRARED TRIPLET LINES; NEGATIVE HYDROGEN-ION; SOLAR-TYPE STARS; EFFECTIVE TEMPERATURES; ANGULAR DIAMETERS; GIANT STARS; II LINES; CALIBRATION; ARCTURUS; PHOTOMETRY
Identifiers
URN: urn:nbn:se:uu:diva-85372OAI: oai:DiVA.org:uu-85372DiVA: diva2:113280
Note
Addresses: EUROPEAN SO OBSERV, SANTIAGO 19, CHILE. STERREWACHT LEIDEN, 2300 RA LEIDEN, NETHERLANDS. ASTRON OBSERV, S-75120 UPPSALA, SWEDEN.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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