Nature of the two modes in the type II bursts of MXB 1730-335
Journal Article
·
· Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:6214021
A Monte Carlo simulation is performed to show that the existence of two modes of type II bursts in the Rapid Burster MXB 1730-335 can be attributed in a natural way to accretion onto either or both magnetic poles of a neutron star rotating with a period of about 250 sec.
- Research Organization:
- Institute for Space Research, USSR Academy of Sciences, Moscow
- OSTI ID:
- 6214021
- Journal Information:
- Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 8:4; ISSN SALED
- Country of Publication:
- United States
- Language:
- English
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Sun Jan 14 23:00:00 EST 1979
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OSTI ID:6326429
Some further information on the rapid burster MXB 1730--335
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OSTI ID:7112474
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· Astrophys. J.; (United States)
·
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Related Subjects
640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCRETION DISKS
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
ELECTROMAGNETIC PULSES
ELECTROMAGNETIC RADIATION
IONIZING RADIATIONS
MAGNETIC FIELDS
MODULATION
MONTE CARLO METHOD
MOTION
NEUTRON STARS
OSCILLATION MODES
PULSES
RADIATIONS
ROTATION
STARS
X RADIATION
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCRETION DISKS
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
ELECTROMAGNETIC PULSES
ELECTROMAGNETIC RADIATION
IONIZING RADIATIONS
MAGNETIC FIELDS
MODULATION
MONTE CARLO METHOD
MOTION
NEUTRON STARS
OSCILLATION MODES
PULSES
RADIATIONS
ROTATION
STARS
X RADIATION