Gamma-ray flare activity from PSR B1259-63 during 2014 Periastron Passage and comparison to its 2010 passage
Journal Article
·
· The Astrophysical Journal (Online)
- Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology; SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Naval Research Lab. (NRL), Washington, DC (United States). Space Science Division
- Inst. of Space Sciences (IEEC-CSIC, Barcelona (Spain)
- NASA Ames Research Center (ARC), Moffett Field, Mountain View, CA (United States)
- Inst. of Space Sciences (IEEC-CSIC), Barcelona (Spain); Catalan Inst. for Research and Advanced Studies (ICREA), Barcelona (Spain)
- Dublin City Univ. (Ireland); Dublin Inst. for Advanced Studies (Ireland). School of Cosmic Physics
PSR B1259–63/LS 2883 is a gamma-ray binary system containing a radio pulsar in a highly elliptical ~3.4-year orbit around a Be star. In its 2010 periastron passage, multiwavelength emission from radio to TeV was observed, as well as an unexpected GeV flare measured by the Fermi Large Area Telescope (LAT). We report the results of LAT monitoring of PSR B1259–63 during its most recent 2014 periastron passage. We also compare the gamma-ray behavior in this periastron with the former in 2010 and find that PSR B1259–63 shows a recurrent GeV flare. Furthermore, the similarities and differences in the phenomenology of both periastron passages are discussed.
- Research Organization:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC02-76SF00515
- OSTI ID:
- 1354903
- Journal Information:
- The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 811; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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