Physical parameters of the continuum emission layer of Mira-type stars. I. Spectrophotometric temperatures

Details Physical parameters of the continuum emission layer of Mira-type stars. I. Spectrophotometric temperatures Physical parameters of the continuum emission layer of Mira-type stars. I. Spectrophotometric temperatures

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap.....50..341r&link_type=abstract

Astrophysics, Volume 50, Issue 3, pp.341-350

Astronomy and Astrophysics

Astrophysics

Stars, Spectrophotometry, Variability

Scientific paper

The spectrophotometric temperatures of five Mira-type variable stars are determined using observations in the Pulkovo spectrophotometric data base in the range from 320 1080 nm. All the resulting temperatures are below the effective temperatures of stars in the corresponding subclasses. Near the brightness maximum, the temperatures are found to be lower with increasing separation in time from the maximum.

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