DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: The first full orbit of η Carinae seen by Fermi

Abstract

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 alongmore » 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.« less

Authors:
 [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)
Publication Date:
Research Org.:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1355158
Grant/Contract Number:  
AC02-76SF00515
Resource Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 577; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; gamma rays: stars; methods: data analysis; stars: individual: η Carinae

Citation Formats

Reitberger, Klaus, Reimer, A., Reimer, O., and Takahashi, H. The first full orbit of η Carinae seen by Fermi. United States: N. p., 2015. Web. doi:10.1051/0004-6361/201525726.
Reitberger, Klaus, Reimer, A., Reimer, O., & Takahashi, H. The first full orbit of η Carinae seen by Fermi. United States. https://doi.org/10.1051/0004-6361/201525726
Reitberger, Klaus, Reimer, A., Reimer, O., and Takahashi, H. Fri . "The first full orbit of η Carinae seen by Fermi". United States. https://doi.org/10.1051/0004-6361/201525726. https://www.osti.gov/servlets/purl/1355158.
@article{osti_1355158,
title = {The first full orbit of η Carinae seen by Fermi},
author = {Reitberger, Klaus and Reimer, A. and Reimer, O. and Takahashi, H.},
abstractNote = {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.},
doi = {10.1051/0004-6361/201525726},
journal = {Astronomy and Astrophysics},
number = ,
volume = 577,
place = {United States},
year = {Fri May 08 00:00:00 EDT 2015},
month = {Fri May 08 00:00:00 EDT 2015}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record

Citation Metrics:
Cited by: 32 works
Citation information provided by
Web of Science

Save / Share:

Works referenced in this record:

High-Energy Particle Transport in Three-Dimensional Hydrodynamic Models of Colliding-Wind Binaries
journal, February 2014


Super-Hard X-Ray Emission from η Carinae Observed with Suzaku
journal, August 2009

  • Sekiguchi, Akiko; Tsujimoto, Masahiro; Kitamoto, Shunji
  • Publications of the Astronomical Society of Japan, Vol. 61, Issue 4
  • DOI: 10.1093/pasj/61.4.629

Radio, X-ray, and γ-ray emission models of the colliding-wind binary WR 140
journal, October 2006


Gamma-ray follow-up studies on η Carinae
journal, August 2012


High-energy radiation from the massive binary system Eta Carinae
journal, May 2011


η Carinae: a very large hadron collider
journal, December 2010


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 SECOND SOURCE CATALOG
journal, March 2012

  • Nolan, P. L.; Abdo, A. A.; Ackermann, M.
  • The Astrophysical Journal Supplement Series, Vol. 199, Issue 2
  • DOI: 10.1088/0067-0049/199/2/31

The Likelihood Analysis of EGRET Data
journal, April 1996

  • Mattox, J. R.; Bertsch, D. L.; Chiang, J.
  • The Astrophysical Journal, Vol. 461
  • DOI: 10.1086/177068

Particle Acceleration in the Expanding Blast wave of η Carina'S Great Eruption of 1843
journal, July 2010


Particle acceleration and nonthermal radio emission in binaries of early-type stars
journal, January 1993

  • Eichler, D.; Usov, V.
  • The Astrophysical Journal, Vol. 402
  • DOI: 10.1086/172130

FERMI LARGE AREA TELESCOPE OBSERVATION OF A GAMMA-RAY SOURCE AT THE POSITION OF ETA CARINAE
journal, October 2010


Detection of Gamma-Ray Emission from the Eta-Carinae Region
journal, June 2009


Constraints on decreases in η Carinae's mass-loss from 3D hydrodynamic simulations of its binary colliding winds
journal, October 2013

  • Madura, T. I.; Gull, T. R.; Okazaki, A. T.
  • Monthly Notices of the Royal Astronomical Society, Vol. 436, Issue 4
  • DOI: 10.1093/mnras/stt1871

Simulating Three-Dimensional Nonthermal High-Energy Photon Emission in Colliding-Wind Binaries
journal, June 2014


X-Ray Monitoring of η Carinae: Variations on a Theme
journal, April 2005

  • Corcoran, M. F.
  • The Astronomical Journal, Vol. 129, Issue 4
  • DOI: 10.1086/428756

THE FERMI LARGE AREA TELESCOPE ON ORBIT: EVENT CLASSIFICATION, INSTRUMENT RESPONSE FUNCTIONS, AND CALIBRATION
journal, October 2012

  • Ackermann, M.; Ajello, M.; Albert, A.
  • The Astrophysical Journal Supplement Series, Vol. 203, Issue 1
  • DOI: 10.1088/0067-0049/203/1/4

Hard X-ray emission from η Carinae
journal, December 2007


Understanding the X-Ray Flaring from η Carinae
journal, November 2009


Works referencing / citing this record:

Fermi Large Area Telescope Fourth Source Catalog
journal, March 2020

  • Abdollahi, S.; Acero, F.; Ackermann, M.
  • The Astrophysical Journal Supplement Series, Vol. 247, Issue 1
  • DOI: 10.3847/1538-4365/ab6bcb

Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae
journal, July 2018

  • Hamaguchi, Kenji; Corcoran, Michael F.; Pittard, Julian M.
  • Nature Astronomy, Vol. 2, Issue 9
  • DOI: 10.1038/s41550-018-0505-1

Modelling the interaction between relativistic and non-relativistic winds in binary pulsar systems: strong magnetization of the pulsar wind
journal, October 2019

  • Bogovalov, S. V.; Khangulyan, D.; Koldoba, A.
  • Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 3
  • DOI: 10.1093/mnras/stz2815

Extended VHE $\gamma$-Ray Emission Towards SGR1806-20, LBV1806-20, and Stellar Cluster Cl*1806-20
text, January 2017

  • Abdalla, H.; Abramowski, A.; Aharonian, F.
  • Deutsches Elektronen-Synchrotron, DESY, Hamburg
  • DOI: 10.3204/pubdb-2017-11577

Colliding-wind binary systems: Diffusive shock acceleration and non-thermal emission
text, January 2019


Extended VHE γ -ray emission towards SGR1806−20, LBV 1806−20, and stellar cluster Cl* 1806−20
journal, April 2018


Embedded star clusters as sources of high-energy cosmic rays: Modelling and constraints
journal, June 2016


Fermi Large Area Telescope Fourth Source Catalog
text, January 2020

  • Abdollahi, S.; Acero, F.; Ackermann, Markus
  • Deutsches Elektronen-Synchrotron, DESY, Hamburg
  • DOI: 10.3204/pubdb-2020-01400

Colliding-wind binary systems: diffusive shock acceleration and non-thermal emission
journal, April 2020

  • Pittard, J. M.; Vila, G. S.; Romero, G. E.
  • Monthly Notices of the Royal Astronomical Society, Vol. 495, Issue 2
  • DOI: 10.1093/mnras/staa1099

Proton Acceleration in Colliding Stellar Wind Binaries
journal, January 2019

  • Grimaldo, Emanuele; Reimer, Anita; Kissmann, Ralf
  • The Astrophysical Journal, Vol. 871, Issue 1
  • DOI: 10.3847/1538-4357/aaf6ee

Investigation of the WR 11 field at decimeter wavelengths
text, January 2019


Investigation of the WR 11 field at decimeter wavelengths
journal, May 2019


Fermi Large Area Telescope Fourth Source Catalog
collection, January 2020