FERMI LARGE AREA TELESCOPE OBSERVATION OF SUPERNOVA REMNANT S147

Katsuta J, Uchiyama Y, Tanaka T, Tajima H, Bechtol K, Funk S, Lande J, Ballet J, Hanabata Y, Lemoine-Goumard M, Takahashi T (2012)


Publication Type: Journal article

Publication year: 2012

Journal

Book Volume: 752

Journal Issue: 2

DOI: 10.1088/0004-637X/752/2/135

Abstract

We present an analysis of gamma-ray data obtained with the Large Area Telescope on board the Fermi Gamma-ray Space Telescope in the region around supernova remnant (SNR) S147 (G180.0-1.7). A spatially extended gamma-ray source detected in an energy range of 0.2-10 GeV is found to coincide with SNR S147. We confirm its spatial extension at >5 sigma confidence level. The gamma-ray flux is (3.8 +/- 0.6) x 10(-8) photons cm(-2) s(-1), corresponding to a luminosity of 1.3 x 10(34) (d/1.3 kpc)(2) erg s(-1) in this energy range. The gamma-ray emission exhibits a possible spatial correlation with the prominent Ha filaments of SNR S147. There is no indication that the gamma-ray emission comes from the associated pulsar PSR J0538 + 2817. The gamma-ray spectrum integrated over the remnant is likely dominated by the decay of neutral pi mesons produced through the proton-proton collisions in the filaments. The reacceleration of the pre-existing cosmic rays and subsequent adiabatic compression in the filaments is sufficient to provide the energy density required of high-energy protons.

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APA:

Katsuta, J., Uchiyama, Y., Tanaka, T., Tajima, H., Bechtol, K., Funk, S.,... Takahashi, T. (2012). FERMI LARGE AREA TELESCOPE OBSERVATION OF SUPERNOVA REMNANT S147. Astrophysical Journal, 752(2). https://dx.doi.org/10.1088/0004-637X/752/2/135

MLA:

Katsuta, J., et al. "FERMI LARGE AREA TELESCOPE OBSERVATION OF SUPERNOVA REMNANT S147." Astrophysical Journal 752.2 (2012).

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