Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-05-23
Astronomy and Astrophysics
Astrophysics
13 pages, 4 figures, submitted to ApJ
Scientific paper
10.1086/342306
Using the Chandra/ACIS-I detector, we have identified an X-ray source (CXOU 132619.7-472910.8) in the globular cluster NGC 5139 with a thermal spectrum identical to that observed from transiently accreting neutron stars in quiescence. The absence of intensity variability on timescales as short as 4 seconds (< 25% rms variability) and as long as 5 years (<50% variability) supports the identification of this source as a neutron star, most likely maintained at a high effective temperature (approximately 1e6 K) by transient accretion from a binary companion. The ability to spectrally identify quiescent neutron stars in globular clusters (where the distance and interstellar column densities are known) opens up new opportunities for precision neutron star radius measurements.
Bildsten Lars
Brown Edward F.
Pavlov George G.
Rutledge Robert E.
Zavlin Vyacheslav E.
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