We report on submillimetre bolometer observations of the isolated neutron star RX J1856.5−3754 using the Large Apex Bolometer Camera bolometer array on the Atacama Pathfinder Experiment telescope. No cold dust continuum emission peak at the position of RX J1856.5−3754 was detected. The 3σ flux density upper limit of 5 mJy translates into a cold dust mass limit of a few earth masses. We use the new submillimetre limit, together with a previously obtained H-band limit, to constrain the presence of a gaseous, circumpulsar disc. Adopting a simple irradiated disc model, we obtain a mass accretion limit of Graphic and a maximum outer disc radius of ∼1014 cm. By examining the projected proper motion of RX J1856.5−3754, we speculate about a possibl...
We report on observations of the neutron star (NS) residing in the low-mass X-ray binary 1RXS J18040...
Thanks to the high counting statistics provided by a recent XMM-Newton observation of RX J1856.5-375...
International audiencePrevious XMM-Newton observations of the thermally emitting isolated neutron st...
We report on submillimetre bolometer observations of the isolated neutron star RX J1856.5−3754 using...
We discuss efforts to determine the mass, radius, and surface composition of the nearby compact obje...
We present results of the analysis of data collected in 57-ks XMM-Newton and 505-ks Chandra observat...
Recent Chandra observations have convincingly shown that the soft X-ray emission from the isolated n...
Observations of cooling neutron stars allow to measure photospheric radii and to constrain the equat...
We report on a deep optical imaging observation using the Subaru Telescope for a very soft X-ray sou...
The possibility that RX J1856.5–3754 is a compact star whose radiation radius is 3.8–8.2 km was sugg...
RX J1856.5-3754 and RX J0720.4-3125 are the only young isolated radio-quiet neutron stars (NSs) for ...
We show that observations of X-ray pulsing from SAX J1808.4-3658 place a firm upper limit of 13.8 m^...
We show that observations of X-ray pulsing from SAX J1808.4-3658 place a firm upper limit of 13.8m(1...
International audienceWe present continuum high-resolution Submillimeter Array (SMA) observations of...
We show that a survey of equations of state and bservations of X-ray pulsations from SAX J1808.4-365...
We report on observations of the neutron star (NS) residing in the low-mass X-ray binary 1RXS J18040...
Thanks to the high counting statistics provided by a recent XMM-Newton observation of RX J1856.5-375...
International audiencePrevious XMM-Newton observations of the thermally emitting isolated neutron st...
We report on submillimetre bolometer observations of the isolated neutron star RX J1856.5−3754 using...
We discuss efforts to determine the mass, radius, and surface composition of the nearby compact obje...
We present results of the analysis of data collected in 57-ks XMM-Newton and 505-ks Chandra observat...
Recent Chandra observations have convincingly shown that the soft X-ray emission from the isolated n...
Observations of cooling neutron stars allow to measure photospheric radii and to constrain the equat...
We report on a deep optical imaging observation using the Subaru Telescope for a very soft X-ray sou...
The possibility that RX J1856.5–3754 is a compact star whose radiation radius is 3.8–8.2 km was sugg...
RX J1856.5-3754 and RX J0720.4-3125 are the only young isolated radio-quiet neutron stars (NSs) for ...
We show that observations of X-ray pulsing from SAX J1808.4-3658 place a firm upper limit of 13.8 m^...
We show that observations of X-ray pulsing from SAX J1808.4-3658 place a firm upper limit of 13.8m(1...
International audienceWe present continuum high-resolution Submillimeter Array (SMA) observations of...
We show that a survey of equations of state and bservations of X-ray pulsations from SAX J1808.4-365...
We report on observations of the neutron star (NS) residing in the low-mass X-ray binary 1RXS J18040...
Thanks to the high counting statistics provided by a recent XMM-Newton observation of RX J1856.5-375...
International audiencePrevious XMM-Newton observations of the thermally emitting isolated neutron st...