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The first full orbit of η Carinae seen by Fermi

Journal Article · · Astronomy and Astrophysics
 [1];  [2];  [2];  [3]
  1. Leopold-Franzens-Univ. Innsbruck, Innsbruck (Austria)
  2. Leopold-Franzens-Univ. Innsbruck, Innsbruck (Austria); Stanford Univ., Stanford, CA (United States). SLAC National Accelerator Lab.
  3. Hiroshima Univ., Hiroshima (Japan)
The binary system η Carinae has completed its first 5.54 y orbit since the beginning of science operation of the Fermi Large Area Telescope (LAT). We are now able to investigate the high-energy γ-ray source at the position of η Carinae over its full orbital period. By this, we can address and confirm earlier predictions for temporal and spectral variability. Here, newer versions of the LAT datasets, instrument response functions and background models allow for a more accurate analysis. Therefore it is important to re-evaluate the previously analyzed time period along with the new data to further constrain location, spectral shape, and flux time history of the γ-ray source. As a result, we confirm earlier predictions of increasing flux values above 10 GeV toward the next periastron passage. For the most recent part of the data sample, flux values as high as those before the first periastron passage in 2008 are recorded. A comparison of spectral energy distributions around periastron and apastron passages reveals strong variation in the high-energy band. This is due to a second spectral component that is present only around periastron. In conclusion, improved spatial consistency with the γ-ray source at the position of η Carinae along with the confirmation of temporal variability above 10 GeV in conjunction with the orbital period strengthens the argument for unambiguous source identification. Spectral variability provides additional constraints for future modeling of the particle acceleration and γ-ray emission in colliding-wind binary systems.
Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1355158
Journal Information:
Astronomy and Astrophysics, Journal Name: Astronomy and Astrophysics Vol. 577; ISSN 0004-6361
Publisher:
EDP SciencesCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (14)

Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae journal July 2018
Embedded star clusters as sources of high-energy cosmic rays: Modelling and constraints journal June 2016
Extended VHE γ -ray emission towards SGR1806−20, LBV 1806−20, and stellar cluster Cl* 1806−20 journal April 2018
Investigation of the WR 11 field at decimeter wavelengths journal May 2019
Colliding-wind binary systems: diffusive shock acceleration and non-thermal emission journal April 2020
Modelling the interaction between relativistic and non-relativistic winds in binary pulsar systems: strong magnetization of the pulsar wind journal October 2019
Fermi Large Area Telescope Fourth Source Catalog collection January 2020
Extended VHE $\gamma$-Ray Emission Towards SGR1806-20, LBV1806-20, and Stellar Cluster Cl*1806-20 text January 2017
Fermi Large Area Telescope Fourth Source Catalog text January 2020
Proton Acceleration in Colliding Stellar Wind Binaries journal January 2019
Fermi Large Area Telescope Fourth Source Catalog journal March 2020
Investigation of the WR 11 field at decimeter wavelengths 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
Colliding-wind binary systems: Diffusive shock acceleration and non-thermal emission text January 2019

Figures / Tables (5)


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