The energy distributions in spectra of 111 late type stars

Details The energy distributions in spectra of 111 late type stars The energy distributions in spectra of 111 late type stars

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..363b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 363

Astronomy and Astrophysics

Astrophysics

Scientific paper

The energy distributions data in the spectra of 111 late-type stars have been obtained in the spectral range 320-790 nm with the resolution near 3 nm. The observations were completed by means of the stellar scanning spectrophotometer mounted on the 80-cm telescope at the Crimean Astrophysical Observatory. The absolute calibration is based on the energy distribution of Vega published by Hayes (1985).

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