{ "id": "1002.2431", "version": "v1", "published": "2010-02-11T21:02:39.000Z", "updated": "2010-02-11T21:02:39.000Z", "title": "Fermi Discovery of Gamma-ray Emission from the Globular Cluster Terzan 5", "authors": [ "A. K. H. Kong", "C. Y. Hui", "K. S. Cheng" ], "comment": "4 pages, 2 figures; accepted for publication in ApJL", "categories": [ "astro-ph.HE" ], "abstract": "We report the discovery of gamma-ray emission from the Galactic globular cluster Terzan 5 using data taken with the Fermi Gamma-ray Space Telescope, from 2008 August 8 to 2010 January 1. Terzan 5 is clearly detected in the 0.5-20 GeV band by Fermi at ~27\\sigma level. This makes Terzan 5 as the second gamma-ray emitting globular cluster seen by Fermi after 47 Tuc. The energy spectrum of Terzan 5 is best represented by an exponential cutoff power-law model, with a photon index of ~1.9 and a cutoff energy at ~3.8 GeV. By comparing to 47 Tuc, we suggest that the observed gamma-ray emission is associated with millisecond pulsars, and is either from the magnetospheres or inverse Compton scattering between the relativistic electrons/positrons in the pulsar winds and the background soft photons from the Galactic plane. Furthermore, it is suggestive that the distance to Terzan 5 is less than 10 kpc and > 10 GeV photons can be seen in the future.", "revisions": [ { "version": "v1", "updated": "2010-02-11T21:02:39.000Z" } ], "analyses": { "keywords": [ "gamma-ray emission", "fermi discovery", "second gamma-ray emitting globular cluster", "exponential cutoff power-law model", "fermi gamma-ray space telescope" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/712/1/L36", "journal": "The Astrophysical Journal", "year": 2010, "month": "Mar", "volume": 712, "number": 1 }, "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable", "inspire": 845767, "adsabs": "2010ApJ...712L..36K" } } }