The long-period x-ray pulsar 3U 0900--40 as a neutron star with an abnormally strong magnetic field
Journal Article
·
· Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:7335492
The observed pulsation period of the binary x-ray source 3U 0900--40 can only be explained if the neutron star has a magnetic-field strength Happrox. =10/sup 14/--10/sup 15/ G. (AIP)
- Research Organization:
- Shternberg Astronomical Institute, Moscow
- OSTI ID:
- 7335492
- Journal Information:
- Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 1:6; ISSN SALED
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BINARY STARS
COSMIC RADIO SOURCES
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
ELECTROMAGNETIC RADIATION
IONIZING RADIATIONS
MAGNETIC FIELDS
NEUTRON STARS
PULSARS
RADIATIONS
STAR ACCRETION
STAR EVOLUTION
STARS
STELLAR WINDS
X RADIATION
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BINARY STARS
COSMIC RADIO SOURCES
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
ELECTROMAGNETIC RADIATION
IONIZING RADIATIONS
MAGNETIC FIELDS
NEUTRON STARS
PULSARS
RADIATIONS
STAR ACCRETION
STAR EVOLUTION
STARS
STELLAR WINDS
X RADIATION