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[en] Spectra covering the 7-23 μm region of the M2Ia star α Orionis have been obtained with the IRAS Low Resolution Spectrometer. These, together with IRAS photometric data and previously published microwave data, have been used to develop a model of the star's outer atmosphere and circumstellar shell. (author)
Journal
Monthly Notices of the Royal Astronomical Society; ISSN 0035-8711; 
; CODEN MNRAA; v. 224(2); p. 335-348
; CODEN MNRAA; v. 224(2); p. 335-348