Aluminum Oxide in Mira During the 1998 Maximum

Details Aluminum Oxide in Mira During the 1998 Maximum Aluminum Oxide in Mira During the 1998 Maximum

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.6604g&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #66.04; Bulletin of the American Astronomical Society, Vol. 31, p.929

Astronomy and Astrophysics

Astronomy

Scientific paper

The long period variable star Mira was monitored at least once a month from October 1998 through maximum light in December 1998 to the end of February 1999. The 1.88m telescope of the David Dunlap Observatory was used with the Cassegrain spectrograph and Thompson 1024 x 1024 CCD detector. The resolution was 0.2A per pixel, and the wavelength ranges covered monthly were: 3900-4500A (H, Ca I, TiO, AlO), 4400-5000A (H, TiO, AlO), 6200-6800A (H, TiO, VO), 7700-8300A (O I, TiO, VO). The data sets were reduced using IRAF. The temperature, luminosity, aluminum strength, and aluminum oxide strength of the relatively faint maximum of December 1998 will be illustrated and discussed.

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