We raise the possibility that the very dense, compact companion of PSR J1719-1438, which has a Jupiter-like mass, is an exotic quark object rather than a light helium or carbon white dwarf. The exotic hypothesis naturally explains some of the observed features, and provides quite strong predictions for this system, to be confirmed or refuted in feasible future studies
We report on Keck optical BVRI images and spectroscopy of the companion of the binary millisecond pu...
We report on the identification of a near-infrared counterpart to the massive (> 11 M) binary com...
We have used phase-resolved high-resolution images and low-resolution spectra taken at the ESO Very ...
We raise the possibility that the very dense, compact companion of PSR J1719-1438, which has a Jupit...
Abstract We raise the possibility that the very dense, compact companion of PSR J1719–1438, which ha...
We present optical and near-infrared observations with Keck of the binary millisecond pulsar PSR J07...
The recycled pulsar PSR J2222-0137 is one of the closest known neutron stars (NSs) with a parallax d...
Most millisecond pulsars with low-mass companions are in systems with either helium-core white dwarf...
We report the identification of the optical counterpart to the companion of the millisecond pulsar J...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
are now also known to be highly inclined ( 2). Some are even retrograde, orbiting in a direction cou...
We report on the discovery of a binary pulsar, PSR J1740-3052, during the Parkes multibeam survey. T...
Abstract We report the identification of the optical counterpart to the companion of the millisecond...
The hierarchical triple system PSR J0337+1715 offers an unprecedented laboratory to study secular ev...
We report on Keck optical BVRI images and spectroscopy of the companion of the binary millisecond pu...
We report on the identification of a near-infrared counterpart to the massive (> 11 M) binary com...
We have used phase-resolved high-resolution images and low-resolution spectra taken at the ESO Very ...
We raise the possibility that the very dense, compact companion of PSR J1719-1438, which has a Jupit...
Abstract We raise the possibility that the very dense, compact companion of PSR J1719–1438, which ha...
We present optical and near-infrared observations with Keck of the binary millisecond pulsar PSR J07...
The recycled pulsar PSR J2222-0137 is one of the closest known neutron stars (NSs) with a parallax d...
Most millisecond pulsars with low-mass companions are in systems with either helium-core white dwarf...
We report the identification of the optical counterpart to the companion of the millisecond pulsar J...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
are now also known to be highly inclined ( 2). Some are even retrograde, orbiting in a direction cou...
We report on the discovery of a binary pulsar, PSR J1740-3052, during the Parkes multibeam survey. T...
Abstract We report the identification of the optical counterpart to the companion of the millisecond...
The hierarchical triple system PSR J0337+1715 offers an unprecedented laboratory to study secular ev...
We report on Keck optical BVRI images and spectroscopy of the companion of the binary millisecond pu...
We report on the identification of a near-infrared counterpart to the massive (> 11 M) binary com...
We have used phase-resolved high-resolution images and low-resolution spectra taken at the ESO Very ...