Propeller effect in two brightest transient X-ray pulsars: 4U 0115+63 and V 0332+53
arXiv:1602.03177 · doi:10.1051/0004-6361/201628236
Abstract
We present the results of the monitoring programmes performed with the Swift/XRT telescope and aimed specifically to detect an abrupt decrease of the observed flux associated with a transition to the propeller regime in two well known X-ray pulsars 4U 0115+63 and V 0332+53 during their giant outbursts in 2015. Such transitions were detected at the threshold luminosities of erg s and erg s for 4U 0115+63 and V 0332+53, respectively. Spectra of the sources are shown to be significantly softer during the low state. In both sources, the accretion at rates close to the aforementioned threshold values briefly resumes during the periastron passage following the transition into propeller regime. The strength of the dipole component of the magnetic field required to inhibit the accretion agrees well with estimates based on the position of the cyclotron lines in their spectra, thus excluding presence of a strong multipole component of the magnetic field in the vicinity of the neutron star.
7 pages, 4 figures, accepted by A&A
References in corpus (14)
- An Ultraluminous X-ray Source Powered by An Accreting Neutron Star
- Thermal and Bulk Comptonization in Accretion-Powered X-Ray Pulsars
- The critical accretion luminosity for magnetized neutron stars
- "Propeller" Regime of Disk Accretion to Rapidly Rotating Stars
- 4U 0115+63 from RXTE and INTEGRAL Data: Pulse Profile and Cyclotron Line Energy
- The ultra luminous X-ray source NuSTAR J095551+6940.8: A magnetar in a high mass X-ray binary
- On the dependence of the X-ray continuum variations with luminosity in accreting X-ray pulsars
- An ultraluminous nascent millisecond pulsar
- The return to quiescence of Aql X-1 following the 2010 outburst
- Swift observations of SAX J1808.4-3658: monitoring the return to quiescence
- Magnetic fields of neutron stars in X-ray binaries
- GK Per and EX Hya: Intermediate polars with small magnetospheres
- GRO J1744-28: an intermediate B-field pulsar in a low mass X-ray binary
- Supergiant, fast, but not so transient 4U 1907+09
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