Published June 1982 | Version v1
Journal article Metadata-only

Why are X-ray pulsars not observed coupled with Wolf-Rayet stars stars

Creators

  • 1. Moskovskij Gosudarstvennyj Univ. (USSR). Gosudarstvennyj Astronomicheskij Inst. ''GAISh''

Description

The peculiarities of an accretion by neutron stars in binary systems with the other component being a Wolf-Rayet star is analysed. It is shown that an X-ray pulsar phenomenon in the systems considered can occur but under specific conditions

Additional details

Additional titles

Original title (Russian)
Почему не наблюдаюця рентгеновские пульсары в парах со звездами Вольфа-Райе со звездами Вольфа-Райе

Publishing Information

Journal Title
Pis'ma Astron. Zh.
Journal Volume
8
Journal Issue
6
Series
Pis'ma Astron. Zh.
Journal Page Range
358-361
ISSN
0320-0108

INIS

Country of Publication
Russian Federation
Country of Input or Organization
USSR
INIS RN
14726368
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BINARY STARS; COSMIC X-RAY SOURCES; NEUTRON STARS; PULSARS; STAR ACCRETION; WOLF-RAYET STARS
Descriptors DEC
COSMIC RADIO SOURCES; COSMIC RAY SOURCES; MAIN SEQUENCE STARS; STAR EVOLUTION; STARS

Optional Information

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