Exosat observations of 4U 1705-44 - Type I bursts and persistent emission
Journal Article
·
· Astrophys. J.; (United States)
During four Exosat observations, the bright galactic X-ray source 4U 1705-44 exhibited persistent emission variations from 1.3 to 10.7 x 10 to the -9th ergs/sq cm per sec in the 1-20 keV band. Type I X-ray bursts have been detected from this source whose properties correlate with source intensity. The burst shape changed with increasing intensity from a slow burst profile with a decay time of 100 sec to a feast profile with a decay time of 25 sec. The spectrum during maximum was best-fitted by a two-component model involving a blackbody together with a Boltzmann-Wien law, and an additional iron K emission line. 28 references.
- Research Organization:
- Max-Planck-Institut fuer Extraterrestrische Physik, Garching, Germany, F.R.; EXOSAT Observatory, Noordwijk, Netherlands
- OSTI ID:
- 5477537
- Journal Information:
- Astrophys. J.; (United States), Vol. 323
- Country of Publication:
- United States
- Language:
- English
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Journal Article
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Sat Apr 01 00:00:00 EST 1989
· Astrophys. J.; (United States)
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OSTI ID:5477537
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Detection of a strong excess noise component in the low state of 4U 1705-44
Journal Article
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Mon May 01 00:00:00 EDT 1989
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OSTI ID:5477537
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OSTI ID:5477537
Related Subjects
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC X-RAY SOURCES
VARIATIONS
BINARY STARS
BLACKBODY RADIATION
COSMIC X-RAY BURSTS
EMISSION SPECTRA
MILKY WAY
RADIANT FLUX DENSITY
COSMIC RAY SOURCES
ELECTROMAGNETIC RADIATION
FLUX DENSITY
GALAXIES
RADIATIONS
SPECTRA
STARS
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources
GENERAL PHYSICS
COSMIC X-RAY SOURCES
VARIATIONS
BINARY STARS
BLACKBODY RADIATION
COSMIC X-RAY BURSTS
EMISSION SPECTRA
MILKY WAY
RADIANT FLUX DENSITY
COSMIC RAY SOURCES
ELECTROMAGNETIC RADIATION
FLUX DENSITY
GALAXIES
RADIATIONS
SPECTRA
STARS
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources