We have monitored the quasi-persistent neutron-star X-ray transient MXB 1659-29 in quiescence using Chandra. The purpose of our observations was to monitor the quiescent behavior of the source after its last prolonged outburst episode and to study the cooling curve of the neutron star in this system. We discuss the results obtained and how they constrain the properties of the neutron star in MXB 1659-29
We report on XMM-Newton observations performed on 2001 September 13-14 of the neutron star X-ray tra...
The quasi-persistent neutron star X-ray transient and eclipsing binary EXO 0748-676 recently started...
Monitoring the cooling of neutron-star crusts heated during accretion outbursts allows us to infer t...
We have observed the quasi-persistent neutron-star X-ray transient and eclipsing binary MXB 1659-29 ...
After almost 2.5 yr of actively accreting, the neutron star X-ray transient and eclipsing binary MXB...
The quasi-persistent neutron star low-mass X-ray binary MXB 1659-29 went into quiescence in 2001, an...
The quasi-persistent neutron star low-mass X-ray binary MXB 1659–29 went into quiescence in 2001, an...
We present Chandra and XMM-Newton X-ray observations that monitor the neutron star cooling of the qu...
ABSTRACT We have observed the quasi-persistent neutron star X-ray transient and eclipsing binary MXB...
In quasi-persistent neutron star transients, long outbursts cause the neutron star crust to be heate...
In the past decade the observing of cooling neutron star transients after long-duration (year or lon...
We have monitored the cooling of the neutron star in the transient low-mass X-ray binary XTE J1701-4...
In the past decade the observing of cooling neutron star transients after long-duration (year or lon...
We present the results of continued monitoring of the quiescent neutron star low-mass X-ray binary X...
We present the results of continued monitoring of the quiescent neutron star low-mass X-ray binary X...
We report on XMM-Newton observations performed on 2001 September 13-14 of the neutron star X-ray tra...
The quasi-persistent neutron star X-ray transient and eclipsing binary EXO 0748-676 recently started...
Monitoring the cooling of neutron-star crusts heated during accretion outbursts allows us to infer t...
We have observed the quasi-persistent neutron-star X-ray transient and eclipsing binary MXB 1659-29 ...
After almost 2.5 yr of actively accreting, the neutron star X-ray transient and eclipsing binary MXB...
The quasi-persistent neutron star low-mass X-ray binary MXB 1659-29 went into quiescence in 2001, an...
The quasi-persistent neutron star low-mass X-ray binary MXB 1659–29 went into quiescence in 2001, an...
We present Chandra and XMM-Newton X-ray observations that monitor the neutron star cooling of the qu...
ABSTRACT We have observed the quasi-persistent neutron star X-ray transient and eclipsing binary MXB...
In quasi-persistent neutron star transients, long outbursts cause the neutron star crust to be heate...
In the past decade the observing of cooling neutron star transients after long-duration (year or lon...
We have monitored the cooling of the neutron star in the transient low-mass X-ray binary XTE J1701-4...
In the past decade the observing of cooling neutron star transients after long-duration (year or lon...
We present the results of continued monitoring of the quiescent neutron star low-mass X-ray binary X...
We present the results of continued monitoring of the quiescent neutron star low-mass X-ray binary X...
We report on XMM-Newton observations performed on 2001 September 13-14 of the neutron star X-ray tra...
The quasi-persistent neutron star X-ray transient and eclipsing binary EXO 0748-676 recently started...
Monitoring the cooling of neutron-star crusts heated during accretion outbursts allows us to infer t...
Add to ORKG