Results 101 to 110 of about 111,592 (291)
Internal Heating of Old Neutron Stars: Contrasting Different Mechanisms
, 2010 The thermal emission detected from the millisecond pulsar J0437-4715 is not explained by standard cooling models of neutron stars without a heating mechanism.
Fernandez, Rodrigo +2 more
core +1 more source
Consistency between the luminosity function of resolved millisecond pulsars and the galactic center excess [PDF]
, 2017 Fermi Large Area Telescope data reveal an excess of GeV gamma rays from the direction of the Galactic Center and bulge. Several explanations have been proposed for this excess including an unresolved population of millisecond pulsars (MSPs) and self ...
H. Ploeg +3 more
semanticscholar +1 more source
Heavy Elements and Electromagnetic Transients from Neutron Star Mergers
Annalen der Physik, Volume 536, Issue 2, February 2024.Astro‐(physics) has made major leaps forward through the combined information provided by both gravitational waves and electromagnetic emission from the first detected neutron star merger event. This review provides an up‐to‐date overview of today's understanding of neutron star mergers and their electromagnetic emission and it discusses possible ...
Stephan Rosswog, Oleg Korobkin
wiley +1 more source
White Noises on Different Stokes Components of Six Millisecond Pulsars
The Astrophysical JournalWe presented measurements of jitter noise and radiometer noise for the Stokes parameters I , L , and V in six millisecond pulsars from the International Pulsar Timing Array sample, based on FAST observations.
S. N. Sun, N. Wang, W. M. Yan
doaj +1 more source
Eight new MSPs in NGC 6440 and NGC 6441
, 2007 We report the discovery of five new millisecond pulsars in the globular cluster NGC 6440 and three new ones in NGC 6441; each cluster has one previously known pulsar. Four of the new pulsars are found in binary systems.
A. Cumming +10 more
core +1 more source
THE NANOGRAV NINE-YEAR DATA SET: MASS AND GEOMETRIC MEASUREMENTS OF BINARY MILLISECOND PULSARS [PDF]
, 2016 We analyze 24 binary radio pulsars in the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) nine-year data set. We make 14 significant measurements of the Shapiro delay, including new detections in four pulsar-binary systems (PSRs ...
E. Fonseca +19 more
semanticscholar +1 more source
A Multiwavelength View of the Neutron Star Binary 1FGL J1417.7–4402: A Progenitor to Canonical Millisecond Pulsars [PDF]
Astrophysical Journal, 2018 The Fermi γ-ray source 1FGL J1417.7–4407 (J1417) is a compact X-ray binary with a neutron star primary and a red giant companion in a ∼5.4 days orbit. This initial conclusion, based on optical and X-ray data, was confirmed when a 2.66 ms radio pulsar was
S. Swihart +8 more
semanticscholar +1 more source
Accretion-powered millisecond pulsars [PDF]
Advances in Space Research, 2006 I review X-ray observations of accretion-powered millisecond pulsars and current theories for formation of their spectra and pulse profiles.
openaire +2 more sources
Millisecond Pulsars, their Evolution and Applications [PDF]
, 2017 Millisecond pulsars (MSPs) are short-period pulsars that are distinguished from “normal” pulsars, not only by their short period, but also by their very small spin-down rates and high probability of being in a binary system.
R. Manchester
semanticscholar +1 more source
The Mass of a Millisecond Pulsar [PDF]
The Astrophysical Journal, 2005 Abstract not available.
Jacoby, Bryan A. +4 more
openaire +3 more sources