Published January 1986 | Version v1
Journal article

Spectrophotometry of carbon stars

  • 1. Byorakan Astrophysical Observatory

Description

The results are given of the spectrophotometric investigation of 56 carbon stars in the spectral range from 4000 to 6800 A with resolution 3 A. The observed energy distributions of these stars are determined relative to the flux at the wavelength 0 = 5556; they are presented in the form of graphs. The energy distributions have been obtained for the first time for 35 stars. Variation in the line Ba II 4554 A has been found in the spectra of St Cam, UU Aur, and RV Mon. Large changes have taken place in the spectra of RT UMa and SS Vir. It is noted that the spectra of carbon stars have a depression, this being situated in different spectral regions for individual groups of stars

Additional details

Publishing Information

Journal Title
Astrophysics (Engl. Transl.)
Journal Volume
23
Journal Issue
1
Series
Astrophysics (Engl. Transl.).
Journal Page Range
432-439
ISSN
0004-6396
CODEN
ATPYA

Optional Information

Notes
Cover-to-cover translation of Astrofizika (USSR).