Results 91 to 100 of about 3,124 (236)

New millisecond pulsars in globular clusters

AIP Conference Proceedings, 2001
Paper presented at the 20th Texas Symposium on Relativistic Astrophysics, 10-15 December 2000 - Austin ...
D'AMICO, NICOLO', POSSENTI A., MANCHESTER R. N., SARKISSIAN J., LYNE A. G., CAMILO F.   +5 more
openaire   +3 more sources

COBIPULSE: A Systematic Search for Compact Binary Millisecond Pulsars

The Astrophysical Journal
We report here the results obtained from a systematic optical photometric survey aimed at finding new compact binary millisecond pulsars (also known as “spiders”): the COmpact BInary PULsar SEarch. We acquired multiband optical images over 1 yr around 33
Marco Turchetta, Manuel Linares, Karri Koljonen, Jorge Casares, Paulo A. Miles-Páez, Pablo Rodríguez-Gil, Tariq Shahbaz, Jordan A. Simpson   +7 more
doaj   +1 more source

GRAVITATIONAL RADIATION FROM ACCRETING MILLISECOND PULSARS

The Eleventh Marcel Grossmann Meeting, 2008
It is widely assumed that the observed reduction of the magnetic field of millisecond pulsars can be connected to the accretion phase during which the pulsar is spun up by mass accretion from a companion. A wide variety of reduction mechanisms have been proposed, including the burial of the field by a magnetic mountain, formed when the accreted matter ...
Vigelius, Matthias, Payne, Donald, Melatos, Andrew   +2 more
openaire   +2 more sources

The optical counterparts of accreting millisecond X-ray pulsars during quiescence [PDF]

, 2009
P. D'Avanzo, S. Campana, J. Casares, S. Covino, G. L. Israel, L. Stella   +5 more
openalex   +1 more source

ePoster

European Journal of Neurology, Volume 32, Issue S1, June 2025.
wiley   +1 more source

Discovery of Four Isolated Millisecond Pulsars

The Astrophysical Journal, 1997
We report the discovery of four isolated millisecond pulsars found as part of the Parkes 436 MHz survey of the southern sky. Three of the pulsars, PSRs J1024-0719, J1744-1134, and J2124-3358, are close to the Sun (d <360 pc) and have very low luminosities, ≲0.5 mJy kpc2. The other, PSR J0711-6830, is of intermediate luminosity.
Bailes, M., Johnston, S., Bell, J. F., Lorimer, D. R., Stappers, B. W., Manchester, R. N., Lyne, A. G., Nicastro, L., D'Amico, N., Gaensler, B. M.   +9 more
openaire   +3 more sources

A binary pulsar in a 53-minute orbit. [PDF]

Nature, 2023
Pan Z, Lu JG, Jiang P, Han JL, Chen HL, Han ZW, Liu K, Qian L, Xu RX, Zhang B, Luo JT, Yan Z, Yang ZL, Zhou DJ, Wang PF, Wang C, Li MH, Zhu M.   +17 more
europepmc   +1 more source

Spin Rates and Magnetic Fields of Millisecond Pulsars [PDF]

, 2004
Frederick K. Lamb, Wenfei Yu
openalex   +1 more source

Orbital spin dynamics of a millisecond pulsar around a massive BH with a general mass quadrupole [PDF]

, 2020
Tom Kimpson, Kinwah Wu, Silvia Zane
openalex   +1 more source

Discovery of three binary millisecond pulsars

The Astrophysical Journal, 1994
We report the discovery of three binary millisecond pulsars in circular orbits with low-mass companions from a continuing survey of the southern sky with the Parkes radio telescope. The three pulsars, PSR J0034-0534, PSR J1045-4509, and PSR J2145-0750 have pulse periods of 1.87, 7.47, and 16.05 ms and orbital periods of 1.6, 4.1, and 6.8 days ...
Bailes, M., Harrison, P. A., Lorimer, D. R., Johnston, S., Lyne, A. G., Manchester, R. N., D'Amico, N., Nicastro, L., Tauris, T. M., Robinson, C.   +9 more
openaire   +3 more sources