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Fermi Large Area Telescope Observation Of A Gamma-Ray Source At The Position Of Eta Carinae

Journal Article · · The Astrophysical Journal
 [1]
  1. Naval Research Lab. (NRL), Washington, DC (United States); et al.
The Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope detected a γ-ray source that is spatially consistent with the location of Eta Carinae. This source has been persistently bright since the beginning of the LAT survey observations (from 2008 August to 2009 July, the time interval considered here). The γ-ray signal is detected significantly throughout the LAT energy band (i.e., up to ~100 GeV). The 0.1-100 GeV energy spectrum is well represented by a combination of a cutoff power-law model (<10 GeV) and a hard power-law component (>10 GeV). The total flux (>100 MeV) is 3.7+0.3 –0.1 × 10–7 photons s–1 cm–2, with additional systematic uncertainties of 10%, and consistent with the average flux measured by AGILE. The light curve obtained by Fermi is consistent with steady emission. Our observations do not confirm the presence of a γ-ray flare in 2008 October, as reported by Tavani et al., although we cannot exclude that a flare lasting only a few hours escaped detection by the Fermi LAT. We also do not find any evidence for γ-ray variability that correlates with the large X-ray variability of Eta Carinae observed during 2008 December and 2009 January. We are thus not able to establish an unambiguous identification of the LAT source with Eta Carinae.
Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
Fermi LAT Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1357519
Alternate ID(s):
OSTI ID: 21467169
Journal Information:
The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 723; ISSN 0004-637X
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae journal July 2018
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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
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Second AGILE catalogue of gamma-ray sources journal June 2019
Overview of non-transient γ -ray binaries and prospects for the Cherenkov Telescope Array journal November 2019
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  • Reitberger, K.; Reimer, O.; Reimer, A.
  • HIGH ENERGY GAMMA-RAY ASTRONOMY: 5th International Meeting on High Energy Gamma-Ray Astronomy, AIP Conference Proceedings https://doi.org/10.1063/1.4772285
conference January 2012
FERMI LARGE AREA TELESCOPE SECOND SOURCE CATALOG journal March 2012
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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
HESS observations of the Carina nebula and its enigmatic colliding wind binary Eta Carinae: HESS observations of the Carina nebula journal June 2012
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
Possible Detection of Gamma-Rays from Epsilon Eridani journal June 2019
Fermi Large Area Telescope Fourth Source Catalog journal March 2020
Refining the associations of the Fermi Large Area Telescope Source Catalogs text January 2015
Phenomenology of gamma-ray emitting binaries preprint January 2019
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
Colliding-wind binary systems: Diffusive shock acceleration and non-thermal emission text January 2019

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