The binary pulsar PSR J1811-1736: evidence of a low amplitude supernova kick

2006/11/13 by A. Corongiu, M. Krämer, M. Kramer +9 · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #Amplitude #Astronomy #Astrophysics #Binary number #Binary pulsar #Gamma-ray bursts and supernovae #Geophysics and Gravity Measurements #Millisecond pulsar #Neutron star #Physics #Pulsar #Pulsars and Gravitational Waves Research #Quantum mechanics #Supernova #astro-ph

paper · pdf · doi:10.1051/0004-6361:20054385

8 pages, 4 figures, accepted for publication on A&A. (Abridged abstract)

openalex publication_date 2006/11/13 · arxiv created 2006/11/14 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05

Abstract

Aims.The binary pulsar PSR J1811-1736 has been identified, since its discovery, as a member of a double neutron star system. Observations of such binary pulsars allow the measurement of general relativistic effects, which in turn lead to information about the orbiting objects, to their binary evolution and, in a few cases, to tests of theories of gravity.

Citations

• Anomalous Scattering of Highly Dispersed Pulsars
• Formation and evolution of binary and millisecond radio pulsars
• The formation of the double pulsar PSR J0737–3039A/B
• The Parkes Multibeam Pulsar Survey - V. Finding binary and millisecond pulsars
• Determination of the Geometry of the PSR B1913+16 System by Geodetic Precession

Cited by

• THE DOUBLE PULSAR: EVIDENCE FOR NEUTRON STAR FORMATION WITHOUT AN IRON CORE-COLLAPSE SUPERNOVA