Add to ORKGWe report the optical discovery of the companion to the 2 M_☉ millisecond pulsar PSR J1614–2230. The optical colors show that the 0.5 M_☉ companion is a 2.2 Gyr old He-CO white dwarf. We infer that M during the accretion phase is <10^(-2), M_(edd). We show that the pulsar was born with a spin close to its current value, well below the rebirth line. The spin-down parameters, the mass of the pulsar, and the age of the system challenge the simple recycling model for the formation of millisecond pulsars
We report on the discovery of the companion star to the millisecond pulsar J1342+2822B in the globul...
We analyse archival optical data on the binary companion to the millisecond pulsar \j1045\ obtained ...
SDSS J091709.55+463821.8 (hereafter J0917+4638) is the lowest surface gravity white dwarf (WD) curre...
The recycled pulsar PSR J2222–0137 is one of the closest known neutron stars (NSs) with a parallax d...
We report on timing observations of the recently discovered binary pulsar PSR J1952+2630 using the A...
none7siWe present the identification of the companion star to the intermediate-mass binary pulsar (P...
Pulsars in close, eccentric binary systems are usually assumed to have another neutron star as a com...
We report on Keck optical BVRI images and spectroscopy of the companion of the binary millisecond pu...
Millisecond pulsars (MSPs) are rapidly spinning neutron stars, with spin periods Ps ≲ 10 ms, which h...
The definitive version can be found at : http://onlinelibrary.wiley.com/ Copyright Wiley-BlackwellPu...
International audienceWe report on photometric and spectroscopic observations of white dwarf compani...
We present optical high-speed photometry of three millisecond pulsars with low-mass (< 0.3M⊙) white ...
We report the detection of a radial velocity companion to SDSS J091709.55+463821.8, the lowest mass ...
The recycled pulsar PSR J2222-0137 is one of the closest known neutron stars (NSs) with a parallax d...
We have measured the radial velocity variation of the white dwarf secondary in the binary system con...
We report on the discovery of the companion star to the millisecond pulsar J1342+2822B in the globul...
We analyse archival optical data on the binary companion to the millisecond pulsar \j1045\ obtained ...
SDSS J091709.55+463821.8 (hereafter J0917+4638) is the lowest surface gravity white dwarf (WD) curre...
The recycled pulsar PSR J2222–0137 is one of the closest known neutron stars (NSs) with a parallax d...
We report on timing observations of the recently discovered binary pulsar PSR J1952+2630 using the A...
none7siWe present the identification of the companion star to the intermediate-mass binary pulsar (P...
Pulsars in close, eccentric binary systems are usually assumed to have another neutron star as a com...
We report on Keck optical BVRI images and spectroscopy of the companion of the binary millisecond pu...
Millisecond pulsars (MSPs) are rapidly spinning neutron stars, with spin periods Ps ≲ 10 ms, which h...
The definitive version can be found at : http://onlinelibrary.wiley.com/ Copyright Wiley-BlackwellPu...
International audienceWe report on photometric and spectroscopic observations of white dwarf compani...
We present optical high-speed photometry of three millisecond pulsars with low-mass (< 0.3M⊙) white ...
We report the detection of a radial velocity companion to SDSS J091709.55+463821.8, the lowest mass ...
The recycled pulsar PSR J2222-0137 is one of the closest known neutron stars (NSs) with a parallax d...
We have measured the radial velocity variation of the white dwarf secondary in the binary system con...
We report on the discovery of the companion star to the millisecond pulsar J1342+2822B in the globul...
We analyse archival optical data on the binary companion to the millisecond pulsar \j1045\ obtained ...
SDSS J091709.55+463821.8 (hereafter J0917+4638) is the lowest surface gravity white dwarf (WD) curre...