 | This article needs additional citations for
verification. (January 2017) |
| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Sagittarius |
| Right ascension | 18h 08m 27.54s [1] |
| Declination | β36° 58′ 44.3″ [1] |
| Apparent magnitude (V) | 16.51 |
| Spectral type | Neutron star |
| Other designations | |
V4580 Sgr, PSR J1808β3658, SWIFT J1808.5β3655, INTREF 881, XTE J1808β369 | |
| Database references | |
| SIMBAD | data |
The first accreting millisecond pulsar discovered in 1998 by the Italian-Dutch BeppoSAX satellite, SAX J1808.4β3658 revealed X-ray pulsations at the 401 Hz neutron star spin frequency when it was observed during a subsequent outburst in 1998 by NASA's RXTE satellite. [2] The neutron star is orbited by a brown dwarf binary companion with a likely mass of 0.05 solar masses, every 2.01 hours. X-ray burst oscillations and quasi-periodic oscillations in addition to coherent X-ray pulsations have been seen from SAX J1808.4-3658, making it a Rosetta stone for interpretation of the timing behavior of low-mass X-ray binaries.
These accreting millisecond X-ray pulsars are thought to be the evolutionary progenitors of recycled radio millisecond pulsars. A total of thirteen accreting millisecond X-ray pulsars have been discovered as of January 2011. Three of them are Intermittent millisecond X-ray pulsars (HETE J1900.1-2455, Aql X-1 and SAX J1748.9-2021), i.e. they emit pulsations sporadically during the outburst.
On 21 August 2019 (UTC; 20 August in the US), Neutron Star Interior Composition Explorer (NICER) spotted the brightest X-ray burst so far observed. [4] It came from SAX J1808.4β3658.
- ^ a b "SAX J1808.4-3658". SIMBAD. Centre de donnΓ©es astronomiques de Strasbourg. Retrieved 15 January 2017.
- ^ Wijnands, Rudy; van der Klis, Michiel (1998). "A millisecond pulsar in an X-ray binary system". Nature. 394 (6691): 344β346. Bibcode: 1998Natur.394..344W. doi: 10.1038/28557. S2CID 4428048.
- ^ Elebert, P.; Reynolds, M. T.; Callanan, P. J.; Hurley, D. J.; Ramsay, G.; Lewis, F.; Russell, D. M.; Nord, B.; Kane, S. R.; Depoy, D. L.; Hakala, P. (May 2009). "Optical spectroscopy and photometry of SAX J1808.4-3658 in outburst". Monthly Notices of the Royal Astronomical Society. 395 (884β894). arXiv: 0901.3991. Bibcode: 2009MNRAS.395..884E. doi: 10.1111/j.1365-2966.2009.14562.x.
- ^ NICER Telescope Spots Brightest X-Ray Burst Ever Observed
 | This variable star–related article is a stub. You can help Wikipedia by expanding it. |
| This article needs additional citations for
verification. (January 2017) |
| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Sagittarius |
| Right ascension | 18h 08m 27.54s [1] |
| Declination | β36° 58′ 44.3″ [1] |
| Apparent magnitude (V) | 16.51 |
| Spectral type | Neutron star |
| Other designations | |
V4580 Sgr, PSR J1808β3658, SWIFT J1808.5β3655, INTREF 881, XTE J1808β369 | |
| Database references | |
| SIMBAD | data |
The first accreting millisecond pulsar discovered in 1998 by the Italian-Dutch BeppoSAX satellite, SAX J1808.4β3658 revealed X-ray pulsations at the 401 Hz neutron star spin frequency when it was observed during a subsequent outburst in 1998 by NASA's RXTE satellite. [2] The neutron star is orbited by a brown dwarf binary companion with a likely mass of 0.05 solar masses, every 2.01 hours. X-ray burst oscillations and quasi-periodic oscillations in addition to coherent X-ray pulsations have been seen from SAX J1808.4-3658, making it a Rosetta stone for interpretation of the timing behavior of low-mass X-ray binaries.
These accreting millisecond X-ray pulsars are thought to be the evolutionary progenitors of recycled radio millisecond pulsars. A total of thirteen accreting millisecond X-ray pulsars have been discovered as of January 2011. Three of them are Intermittent millisecond X-ray pulsars (HETE J1900.1-2455, Aql X-1 and SAX J1748.9-2021), i.e. they emit pulsations sporadically during the outburst.
On 21 August 2019 (UTC; 20 August in the US), Neutron Star Interior Composition Explorer (NICER) spotted the brightest X-ray burst so far observed. [4] It came from SAX J1808.4β3658.
- ^ a b "SAX J1808.4-3658". SIMBAD. Centre de donnΓ©es astronomiques de Strasbourg. Retrieved 15 January 2017.
- ^ Wijnands, Rudy; van der Klis, Michiel (1998). "A millisecond pulsar in an X-ray binary system". Nature. 394 (6691): 344β346. Bibcode: 1998Natur.394..344W. doi: 10.1038/28557. S2CID 4428048.
- ^ Elebert, P.; Reynolds, M. T.; Callanan, P. J.; Hurley, D. J.; Ramsay, G.; Lewis, F.; Russell, D. M.; Nord, B.; Kane, S. R.; Depoy, D. L.; Hakala, P. (May 2009). "Optical spectroscopy and photometry of SAX J1808.4-3658 in outburst". Monthly Notices of the Royal Astronomical Society. 395 (884β894). arXiv: 0901.3991. Bibcode: 2009MNRAS.395..884E. doi: 10.1111/j.1365-2966.2009.14562.x.
- ^ NICER Telescope Spots Brightest X-Ray Burst Ever Observed
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