High-energy γ-rays from globular clusters
- 11 May 2007
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 377 (2) , 920-930
- https://doi.org/10.1111/j.1365-2966.2007.11664.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 31 references indexed in Scilit:
- An Ultracompact X-Ray Binary in the Globular Cluster M15 (NGC 7078)The Astrophysical Journal, 2005
- Search for TeV Emissions from Pulsars in Binary SystemsThe Astrophysical Journal, 2003
- [ITAL]Hubble Space Telescope[/ITAL] Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15. II. Kinematic Analysis and Dynamical ModelingThe Astronomical Journal, 2002
- Regimes of Pulsar Pair Formation and Particle EnergeticsThe Astrophysical Journal, 2002
- Pulsar Polar Cap Heating and Surface Thermal X‐Ray Emission. II. Inverse Compton Radiation Pair FrontsThe Astrophysical Journal, 2002
- Toward Resolving the Crab σ‐Problem: A Linear Accelerator?The Astrophysical Journal, 2002
- Spectral features in gamma-rays expected from millisecond pulsarsMonthly Notices of the Royal Astronomical Society, 2000
- Observations of 20 Millisecond Pulsars in 47 Tucanae at 20 CentimetersThe Astrophysical Journal, 2000
- High-energy emission from the eclipsing millisecond pulsar PSR 1957+20The Astrophysical Journal, 1993
- A new class of radio pulsarsNature, 1982