Published May 1989 | Version v1
Journal article

Radiation power of some antiflare stars in the line Hα

Creators

Description

An investigation has been made of the luminosity in the line Hα of five rapid irregular variables: SV Cep, V 530 Cyg, XY Per, VV Ser, and WW Vul. For these tars, 18 spectra were obtained with the 2.6-m telescope of the Crimean Astrophysical Observatory by means of a slit spectrograph and image intensifier. The luminosity of four stars was found to be in the range Eαe = (0.93-16.1)·1032 erg/sec. In the spectrum of V 530 Cyg no emission was found in the Hα. Variability of the profile and intensities of the Hα emission line is confirmed

Additional details

Publishing Information

Journal Title
Astrophysics (English Translation)
Journal Volume
29
Journal Issue
3
Series
Astrophysics (Engl. Transl.).
Journal Page Range
682-687
ISSN
0004-6396
CODEN
ATPYA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
22032928
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Translation
Descriptors DEI
ABSORPTION SPECTRA; BINARY STARS; BRIGHTNESS; COMPARATIVE EVALUATIONS; EMISSION SPECTRA; HYDROGEN; LINE WIDTHS; LUMINOSITY; PLANCK RADIATION FORMULA; REMOTE SENSING; SPECTROPHOTOMETRY; STELLAR RADIATION; VARIABLE STARS
Descriptors DEC
ELEMENTS; EVALUATION; NONMETALS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; SPECTRA; STARS

Optional Information

Notes
(English). Cover-to-cover Translation of Astrofizika (U.S.S.R). Cover-to-cover translation of Astrofizika (USSR).