Published August 1983 | Version v1
Journal article Metadata-only

On the correlation between Hsub(α) line intensity and SiO maser emission of the long-period variable chi Cygni

Creators

  • 1. Leningradskij Gosudarstvennyj Univ. (USSR)

Description

The results of 1975 and 1978-79 observations of the Hsub(α) emission line in the spectrum of chi Cyg are given. Comparison of the obtained data with the observations of the SiO maser line (J=2-1, ν=1) by Wolff and Carlsson (1982) gives evidences of a correlation between the intensities of Hsub(α) and SiO line

Additional details

Additional titles

Original title (Russian)
О корреляции между интенсивностью линии Хсуб(α) и мазерным SiO-излучением долгопериодической переменной охи Лебедя

Publishing Information

Journal Title
Pis'ma Astron. Zh.
Journal Issue
V. 9(8
Series
Pis'ma Astron. Zh.
ISSN
0320-0108

INIS

Country of Publication
Russian Federation
Country of Input or Organization
USSR
INIS RN
15019798
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Numerical Data
Descriptors DEI
BALMER LINES; EMISSION SPECTRA; EXPERIMENTAL DATA; MICROWAVE RADIATION; STELLAR RADIATION; STIMULATED EMISSION
Descriptors DEC
DATA; ELECTROMAGNETIC RADIATION; EMISSION; ENERGY-LEVEL TRANSITIONS; INFORMATION; NUMERICAL DATA; RADIATIONS; SPECTRA

Optional Information

Notes
For English translation see the journal Soviet Astronomy Letters (USA).