Predictions of Gamma-ray Emission from Globular Cluster Millisecond Pulsars Above 100 MeV
arXiv:0903.3031 · doi:10.1088/0004-637X/696/1/L52
Abstract
The recent Fermi detection of the globular cluster (GC) 47 Tucanae highlighted the importance of modeling collective gamma-ray emission of millisecond pulsars (MSPs) in GCs. Steady flux from such populations is also expected in the very high energy (VHE) domain covered by ground-based Cherenkov telescopes. We present pulsed curvature radiation (CR) as well as unpulsed inverse Compton (IC) calculations for an ensemble of MSPs in the GCs 47 Tucanae and Terzan 5. We demonstrate that the CR from these GCs should be easily detectable for Fermi, while constraints on the total number of MSPs and the nebular B-field may be derived using the IC flux components.
12 pages, 2 figures, accepted for publication in ApJL
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Cited by in corpus (43)
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- Very-high-energy gamma-ray emission from the direction of the Galactic globular cluster Terzan 5
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- MeerKAT discovery of 13 new pulsars in Omega Centauri
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- How the dynamical properties of globular clusters impact their -ray and X-ray emission
- Gamma-rays from millisecond pulsars in Globular Clusters
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- A possible GeV-TeV connection in the direction of the Globular Cluster UKS 1
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- MAGIC observation of Globular Cluster M13 and its millisecond pulsars