On the infrared bands of a A10 related to Mira phenomena

Details On the infrared bands of a A10 related to Mira phenomena On the infrared bands of a A10 related to Mira phenomena

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..54..509m&link_type=abstract

Astrophysics and Space Science, vol. 54, no. 2, Apr. 1978, p. 509-512.

Astronomy and Astrophysics

Astrophysics

Aluminum Oxides, Infrared Spectra, Mira Variables, Stellar Spectrophotometry, Variable Stars, Line Spectra, M Stars, Supergiant Stars, Tables (Data)

Scientific paper

The calculated band positions and intensity factors for the bands of the infrared A-X transition of A10 suggest that an investigation for the infrared bands in the 1 to 5 micron region of the spectra of Mira stars and M supergiants, along with the 'blue-green' (B-X) bands, could provide clues to the Mira phenomena. The need for additional laboratory investigation of the infrared electronic transition is emphasized.

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