Multi-telescope timing of PSR J1518+4904

2008/08/17 by G. H. Janssen, B. W. Stappers, M. Krämer +7 · 3 citations
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #Astronomy #Astrophysics #Context (archaeology) #Geology #Geophysics and Gravity Measurements #Geophysics and Sensor Technology #Gravitation #Neutron star #Physics #Pulsars and Gravitational Waves Research #Telescope #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810076

11 pages, 8 figures, accepted by A&A

arxiv created 2008/08/17 · openalex publication_date 2008/09/11 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/06

Abstract

Context. PSR J1518+4904 is one of only 9 known double neutron star systems. These systems are highly valuable for measuring the masses of neutron stars, measuring the effects of gravity, and testing gravitational theories.

Citations

• Formation of double compact objects
• The Supernova Channel of Super‐AGB Stars
• The Characteristics of Millisecond Pulsar Emission. III. From Low to High Frequencies
• Masses, Parallax, and Relativistic Timing of the PSR J1713+0747 Binary System
• The late stages of evolution of helium star-neutron star binaries and the formation of double neutron star systems
• Formation and evolution of binary and millisecond radio pulsars
• The binary pulsar PSR J1811-1736: evidence of a low amplitude supernova kick
• Testing General Relativity with Pulsar Timing
• Neutron Star Mass Measurements. I. Radio Pulsars

Cited by

• OPTICAL IDENTIFICATION OF He WHITE DWARFS ORBITING FOUR MILLISECOND PULSARS IN THE GLOBULAR CLUSTER 47 TUCANAE
• Precise mass measurements for the double neutron star system J1829+2456
• High braking index pulsar PSR J1640-4631: low-mass neutron star with a large inclination angle?