X-ray observations unveiled various types of radio-silent isolated neutron stars (INSs), phenomenologically very diverse, e.g. the ∼Myr old X-ray-dim INSs (XDINSs) and the ∼kyr old magnetars. Although their phenomenology is much diverse, the similar periods (P = 2–10 s) and magnetic fields (≈1014 G) suggest that XDINSs are evolved magnetars, possibly born from similar populations of supermassive stars. One way to test this hypothesis is to identify their parental star clusters by extrapolating backwards the NS velocity vector in the Galactic potential. By using the information on the age and space velocity of the XDINS RX J1856.5−3754, we computed backwards its orbit in the Galactic potential and searched for its parental stellar cluster by...
The low-mass X-ray binary (LMXB) IGR J17480-2446 in the globular cluster Terzan 5 harbors an 11 Hz a...
The low-mass X-ray binary (LMXB) IGR J17480-2446 in the globular cluster Terzan 5 harbors an 11 Hz a...
We explore the hypothesis that the magnetic fields of neutron stars are of fossil origin. For parame...
X-ray observations unveiled various types of radio-silent isolated neutron stars (INSs), phenomenolo...
X-ray observations unveiled various types of radio-silent isolated neutron stars (INSs), phenomenolo...
Young isolated radio-quiet neutron stars are still hot enough to be detectable at X-ray and optical ...
RX J1856.5-3754 and RX J0720.4-3125 are the only young isolated radio-quiet neutron stars (NSs) for ...
Recent observations show that supergiant fast X-ray transients (SFXTs) spend most of their lifetime ...
Previous XMM-Newton observations of the thermally emitting isolated neutron star RX J1605.3+3249 pro...
Context. The first soft gamma-ray repeater was discovered over three decades ago, and was subsequent...
Context. High-energy observations have unveiled peculiar classes of isolated neutron stars which, at...
Magnetars are regarded as the most magnetized neutron stars in the Universe. Aiming to unveil what k...
Aims. To estimate the compactness of the thermally-emitting isolated neutron star (INS) RX J0720.4−3...
We model populations of isolated neutron stars in order to investigate them as progenitors of dim so...
We report the discovery of an X-ray pulsar in the young, massive Galactic star cluster Westerlund 1....
The low-mass X-ray binary (LMXB) IGR J17480-2446 in the globular cluster Terzan 5 harbors an 11 Hz a...
The low-mass X-ray binary (LMXB) IGR J17480-2446 in the globular cluster Terzan 5 harbors an 11 Hz a...
We explore the hypothesis that the magnetic fields of neutron stars are of fossil origin. For parame...
X-ray observations unveiled various types of radio-silent isolated neutron stars (INSs), phenomenolo...
X-ray observations unveiled various types of radio-silent isolated neutron stars (INSs), phenomenolo...
Young isolated radio-quiet neutron stars are still hot enough to be detectable at X-ray and optical ...
RX J1856.5-3754 and RX J0720.4-3125 are the only young isolated radio-quiet neutron stars (NSs) for ...
Recent observations show that supergiant fast X-ray transients (SFXTs) spend most of their lifetime ...
Previous XMM-Newton observations of the thermally emitting isolated neutron star RX J1605.3+3249 pro...
Context. The first soft gamma-ray repeater was discovered over three decades ago, and was subsequent...
Context. High-energy observations have unveiled peculiar classes of isolated neutron stars which, at...
Magnetars are regarded as the most magnetized neutron stars in the Universe. Aiming to unveil what k...
Aims. To estimate the compactness of the thermally-emitting isolated neutron star (INS) RX J0720.4−3...
We model populations of isolated neutron stars in order to investigate them as progenitors of dim so...
We report the discovery of an X-ray pulsar in the young, massive Galactic star cluster Westerlund 1....
The low-mass X-ray binary (LMXB) IGR J17480-2446 in the globular cluster Terzan 5 harbors an 11 Hz a...
The low-mass X-ray binary (LMXB) IGR J17480-2446 in the globular cluster Terzan 5 harbors an 11 Hz a...
We explore the hypothesis that the magnetic fields of neutron stars are of fossil origin. For parame...