Optical identification of the companion to PSR J1911-5958A, the pulsar binary in the outskirts of NGC 6752
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20031339/pdf
Reference21 articles.
1. The impact of element diffusion on the formation and evolution of helium white dwarf stars
2. An Improved Distortion Solution for theHubble Space Telescope’s WFPC2
3. Optical Positions of ICRF Sources Using UCAC Reference Stars
4. The mass of the neutron star in the binary millisecond pulsar PSR J1012 + 5307
5. The Case of PSR J1911−5958A in the Outskirts of NGC 6752: Signature of a Black Hole Binary in the Cluster Core?
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1. The dominant mechanism(s) for populating the outskirts of star clusters with neutron star binaries;Monthly Notices of the Royal Astronomical Society;2023-11-13
2. PSR J1910–5959A: A rare gravitational laboratory for testing white dwarf models;Astronomy & Astrophysics;2023-03
3. A deep search for faint Chandra X-ray sources, radio sources, and optical counterparts in NGC 6752;Monthly Notices of the Royal Astronomical Society;2021-09-27
4. OPTICAL IDENTIFICATION OF He WHITE DWARFS ORBITING FOUR MILLISECOND PULSARS IN THE GLOBULAR CLUSTER 47 TUCANAE;The Astrophysical Journal;2015-10-09
5. Discovery of near-ultraviolet counterparts to millisecond pulsars in the globular cluster 47 Tucanae;Monthly Notices of the Royal Astronomical Society;2015-09-02
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