Gamma-Ray Emission from Globular Clusters 2Ms-Gc01, Ic 1257, Fsr 1735, Ngc 5904 and 6656
Monthly Notices of the Royal Astronomical Society(2015)
摘要
Globular clusters (GCs) are the oldest stellar systems in the Galaxy, in which millisecond pulsars are widely believed to be the only steady gamma-ray emitters. So far, nine gamma-ray GCs have been identified and a few candidates, such as 2MS-GC01 and IC 1257, have been suggested. In this work, after analysing the publicly available Fermi Large Area Telescope data, we confirm the significant gamma-ray emission from 2MS-GC01 and IC 1257 and report the discovery of gamma-ray emission from NGC 5904 and 6656 within their tidal radii. Also, strong evidence of significant gamma-ray emission is found from FSR 1735. From the observed gamma-ray luminosities, we estimate the numbers of millisecond pulsars that are expected to be present in these GCs.
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关键词
gamma-rays: general,globular clusters: individual: NGC 5904,globular clusters: individual: NGC 6656,globular clusters: individual: FSR 1735,globular clusters: individual: 2MS-GC01,globular clusters: individual: IC 1257
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