Transient Low-Mass X-Ray Binaries in Quiescence
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- Type
- preprint
- Published
- 2000-05-17
- Cited by
- 0
- References
- 50
- Access
- Open access
- OpenAlex
- https://openalex.org/W1538644452
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:118594259
Keywords
Neutron star, Physics, Astrophysics, Pulsar, Black hole (networking)
References
- The surface chemistry of stars. I - Diffusion of heavy ions in white dwarf envelopes. II - Fractionated accretion of interstellar matter
- X-ray emission from cataclysmic variables with accretion disks. II. EUV/Soft x-ray radiation
- The two-hour orbit of a binary millisecond X-ray pulsar
- A millisecond pulsar in an X-ray binary system
- Disk-instability model for soft-X-ray transients containing black holes
- X-ray evidence for white dwarf binaries in globular clusters
- Model atmospheres for low field neutron stars
- The dim inner accretion disk of the quiescent black hole A0620-00
- Black Hole Binaries and X-Ray Transients
- X-ray sources in globular clusters
- The X-Ray Eclipse of the Dwarf Nova HT Cassiopeiae: Results from ASCA and ROSAT HRI Observations
- Coronal X-Ray Emission from the Stellar Companions to Transiently Accreting Black Holes
- X-ray observations of a large sample of cataclysmic variable stars using the Einstein Observatory
- The Disk-Magnetosphere Interaction in the Accretion-powered Millisecond Pulsar SAX J1808.4–3658
- Thermal instability accretion disk model for the X-ray transient A0620-00
- ASCA Observations of Transient X-Ray Sources in Quiescence
- X-Ray Spectra from Neutron Stars Accreting at Low Rates
- Crustal Heating and Quiescent Emission from Transiently Accreting Neutron Stars
- Advection-dominated Flows around Black Holes and the X-Ray Delay in the Outburst of GRO J1655–40
- ASCA Observations of Soft X-Ray Transients in Quiescence : X1608-52 and CEN X-4
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