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Title: DISCOVERY OF HIGH-ENERGY GAMMA-RAY EMISSION FROM THE BINARY SYSTEM PSR B1259-63/LS 2883 AROUND PERIASTRON WITH FERMI

Journal Article · · Astrophysical Journal Letters
 [1]; ; ; ; ; ; ; ; ;  [2];  [3];  [4]; ;  [5]; ;  [6];  [7];  [8];  [9]
  1. Center for Earth Observing and Space Research, College of Science, George Mason University, Fairfax, VA 22030 (United States)
  2. W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305 (United States)
  3. Laboratoire AIM, CEA-IRFU/CNRS/Universite Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette (France)
  4. Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34127 Trieste (Italy)
  5. Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova (Italy)
  6. Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa (Italy)
  7. Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia (Italy)
  8. Dipartimento di Fisica 'M. Merlin' dell'Universita e del Politecnico di Bari, I-70126 Bari (Italy)
  9. Laboratoire Leprince-Ringuet, Ecole polytechnique, CNRS/IN2P3, Palaiseau (France)

We report on the discovery of {>=}100 MeV {gamma}-rays from the binary system PSR B1259-63/LS 2883 using the Large Area Telescope (LAT) on board Fermi. The system comprises a radio pulsar in orbit around a Be star. We report on LAT observations from near apastron to {approx}128 days after the time of periastron, t{sub p} , on 2010 December 15. No {gamma}-ray emission was detected from this source when it was far from periastron. Faint {gamma}-ray emission appeared as the pulsar approached periastron. At {approx}t{sub p} + 30 days, the {>=}100 MeV {gamma}-ray flux increased over a period of a few days to a peak flux 20-30 times that seen during the pre-periastron period, but with a softer spectrum. For the following month, it was seen to be variable on daily timescales, but remained at {approx}(1-4) x 10{sup -6} cm{sup -2} s{sup -1} before starting to fade at {approx}t{sub p} + 57 days. The total {gamma}-ray luminosity observed during this period is comparable to the spin-down power of the pulsar. Simultaneous radio and X-ray observations of the source showed no corresponding dramatic changes in radio and X-ray flux between the pre-periastron and post-periastron flares. We discuss possible explanations for the observed {gamma}-ray-only flaring of the source.

OSTI ID:
21562531
Journal Information:
Astrophysical Journal Letters, Vol. 736, Issue 1; Other Information: DOI: 10.1088/2041-8205/736/1/L11; ISSN 2041-8205
Country of Publication:
United States
Language:
English

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Millisecond Pulsars, their Evolution and Applications journal September 2017
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Refining the origins of the gamma-ray binary 1FGL J1018.6–5856 journal November 2018
Overview of non-transient γ -ray binaries and prospects for the Cherenkov Telescope Array journal November 2019
H.E.S.S. and Fermi -LAT observations of PSR B1259–63/LS 2883 during its 2014 and 2017 periastron passages journal January 2020
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Long-Term Monitoring of the High-Energy γ-Ray Emission from ls i +61°303 and ls 5039 journal March 2012
FERMI LARGE AREA TELESCOPE SECOND SOURCE CATALOG journal March 2012
FERMI LARGE AREA TELESCOPE THIRD SOURCE CATALOG journal June 2015
Observational diversity of magnetized neutron stars journal September 2019
DISCOVERY OF GeV γ-RAY EMISSION FROM PSR B1259–63/LS 2883 journal June 2011
HIGH-ENERGY OBSERVATIONS OF PSR B1259–63/LS 2883 THROUGH THE 2014 PERIASTRON PASSAGE: CONNECTING X-RAYS TO THE GeV FLARE journal December 2014
Multiwavelength observations of the binary system PSR B1259−63/LS 2883 around the 2010–2011 periastron passage journal January 2014
The geometric distance and binary orbit of PSR B1259–63 journal July 2018
On the timing behaviour of PSR B1259–63 under the propeller torque from a transient accretion disc journal February 2018
Modelling the interaction between relativistic and non-relativistic winds in binary pulsar systems: strong magnetization of the pulsar wind journal October 2019
First detection of PSR B1259−63/LS 2883 in the millimeter and submillimeter wavelengths with ALMA journal August 2019
Direct wind accretion and jet launch in binary systems: Wind accretion and jet launch in binary systems journal February 2012
Anisotropic inverse Compton scattering of photons from the circumstellar disc in PSR B1259−63: AIC scattering in PSR B1259−63 journal October 2012
FERMI STUDY OF 5–300 GeV EMISSION FROM THE HIGH-MASS PULSAR BINARY PSR B1259-63/LS 2883 journal August 2016
GeV Detection of HESS J0632+057 journal September 2017
Rapid Flaring in the Galactic-plane Gamma-Ray Transient Fermi J0035+6131 journal July 2018
The Hour-timescale GeV Flares of PSR B1259–63 in 2017 journal August 2018
A Luminous and Highly Variable Gamma-Ray Flare Following the 2017 Periastron of PSR B1259–63/LS 2883 journal August 2018
The Likely Fermi Detection of the Be X-Ray Binary GRO J1008-57 journal September 2019
Evolution of the Extended X-Ray Emission from the PSR B1259–63/LS 2883 Binary in the 2014–2017 Binary Cycle journal September 2019
Probing the Properties of the Pulsar Wind in the Gamma-Ray Binary HESS J0632+057 with NuSTAR and VERITAS Observations journal January 2020
H.E.S.S. observations of the binary system PSR B1259-63/LS 2883 around the 2010/2011 periastron passage text January 2013
Probing the Properties of the Pulsar Wind in the Gamma-Ray Binary HESS J0632+057 with NuSTAR and VERITAS Observations text January 2019
The Neutron Star Zoo journal September 2017
H.E.S.S. and Fermi-LAT observations of PSR B1259-63/LS 2883 during its 2014 and 2017 periastron passages text January 2019
Probing the Properties of the Pulsar Wind in the Gamma-Ray Binary HESS J0632+057 with NuSTAR and VERITAS Observations text January 2020
Discovery of GeV gamma-ray emission from PSR B1259-63/LS 2883 text January 2011
Multi-wavelength observations of the binary system PSR B1259-63/LS 2883 around the 2010-2011 periastron passage text January 2014
Fermi Study of 5-300 GeV emission from the high-mass pulsar binary PSR B1259-63/LS 2883 text January 2016
Millisecond Pulsars, their Evolution and Applications text January 2017
The geometric distance and binary orbit of PSR B1259-63 text January 2018
A Luminous and Highly-variable Gamma-ray Flare Following the 2017 Periastron of PSR B1259-63/LS 2883 text January 2018
Rapid Flaring in the Galactic-plane Gamma-ray Transient Fermi J0035+6131 text January 2018
Overview of non-transient gamma-ray binaries and prospects for the Cherenkov Telescope Array text January 2019
Modelling the interaction between relativistic and non-relativistic winds in binary pulsar systems: strong magnetization of the pulsar wind text January 2019
Probing the Properties of the Pulsar Wind in the Gamma-Ray Binary HESS J0632+057 with NuSTAR and VERITAS Observations text January 2019
H.E.S.S. and Fermi-LAT observations of PSR B1259–63/LS 2883 during its 2014 and 2017 periastron passages text January 2020