Energy distribution in giants and supergiants. (Tereshchenko, 1996)

Details Energy distribution in giants and supergiants. (Tereshchenko, 1996) Energy distribution in giants and supergiants. (Tereshchenko, 1996)

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..80730762t&link_type=abstract

VizieR On-line Data Catalog: J/AZh/73/762. Originally published in: 1996AZh....73..762T; 1996ARep...40..693T

Astronomy and Astrophysics

Astrophysics

Stars: Giant, Energy Distributions

Scientific paper

The energy distributions for 27 giants and supergiants of the M spectral type are presented in the region of 3200-7600Å with the step of 50Å. The observations were made in the Fessenkov Astrophysical institute (Alma-Ata) during 1986-1987 with a spectrophotometer of Seya-Namioka mounted on the 50-cm Cassegrain telescope. The primary standard is Vega with the energy distribution by Hayes (1985IAUS..111..225H). The relative r.m.s. of the results are given in the table3.dat. (3 data files).

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