FERMI LARGE AREA TELESCOPE OBSERVATIONS OF THE SUPERNOVA REMNANT G8.7-0.1 - IN2P3 - Institut national de physique nucléaire et de physique des particules
Journal Articles The Astrophysical Journal Year : 2012

FERMI LARGE AREA TELESCOPE OBSERVATIONS OF THE SUPERNOVA REMNANT G8.7-0.1

Marco Ajello , A. Allafort , Luca Baldini , Jean Ballet (1) , Guido Barbiellini , D. Bastieri , K. Bechtol , R. Bellazzini , B. Berenji , R. D. Blandford , E. D. Bloom , E. Bonamente , A. W. Borgland , J. Bregeon , M. Brigida , Pascal Bruel (2) , R. Buehler , S. Buson , G. A. Caliandro , R. A. Cameron , P. A. Caraveo , J. M. Casandjian (1) , C. Cecchi , E. Charles , A. Chekhtman , S. Ciprini , R. Claus , J. Cohen-Tanugi (3) , S. Cutini , A. de Angelis , F. de Palma , C. D. Dermer , E. Do Couto E Silva , P. S. Drell , A. Drlica-Wagner , R. Dubois , C. Favuzzi , S. J. Fegan (2) , E. C. Ferrara , W. B. Focke , M. Frailis , Y. Fukazawa , Y. Fukui , P. Fusco , F. Gargano , D. Gasparrini , S. Germani , N. Giglietto , P. Giommi , F. Giordano , M. Giroletti , T. Glanzman , G. Godfrey , J. E. Grove , S. Guiriec , D. Hadasch , Y. Hanabata , A. K. Harding , K. Hayashi , E. Hays , R. Itoh , G. Jóhannesson , A. S. Johnson , T. Kamae , H. Katagiri , J. Kataoka , Jürgen Knödlseder (4) , H. Kubo , M. Kuss , J. Lande , L. Latronico , S.-H. Lee , A. M. Lionetto , F. Longo , F. Loparco , M. N. Lovellette , P. Lubrano , M. N. Mazziotta , J. Mehault (3) , P. F. Michelson , T. Mizuno , A. A. Moiseev , C. Monte , M. E. Monzani , A. Morselli , I. V. Moskalenko , S. Murgia , T. Nakamori , M. Naumann-Godo (1) , S. Nishino , P. L. Nolan , J. P. Norris , E. Nuss (3) , M. Ohno , T. Ohsugi , A. Okumura , N. Omodei , E. Orlando , J. F. Ormes , D. Paneque , D. Parent , V. Pelassa (3) , M. Pesce-Rollins , M. Pierbattista (1) , F. Piron (3) , T.A. Porter , S. Rainò , R. Rando , A. Reimer , O. Reimer , T. Reposeur (5) , M. Roth , H. F.-W. Sadrozinski , C. Sgrò , E. J. Siskind , P. D. Smith , G. Spandre , P. Spinelli , D. J. Suson , H. Tajima , H. Takahashi , T. Tanaka , J. G. Thayer , J. B. Thayer , L. Tibaldo , O. Tibolla , D. F. Torres , G. Tosti , A. Tramacere , E. Troja , Y. Uchiyama , T. Uehara , T. L. Usher , J. Vandenbroucke , A. van Etten , V. Vasileiou (3) , G. Vianello , N. Vilchez (4) , V. Vitale , A. P. Waite , P. Wang , B. L. Winer , K. S. Wood , H. Yamamoto , R. Yamazaki , Z. Yang , H. Yasuda , M. Ziegler , S. Zimmer
Marco Ajello
  • Function : Author
A. Allafort
  • Function : Author
Luca Baldini
  • Function : Author
Guido Barbiellini
  • Function : Author
D. Bastieri
  • Function : Author
K. Bechtol
  • Function : Author
R. Bellazzini
  • Function : Author
B. Berenji
  • Function : Author
R. D. Blandford
  • Function : Author
E. D. Bloom
  • Function : Author
E. Bonamente
  • Function : Author
A. W. Borgland
  • Function : Author
J. Bregeon
M. Brigida
  • Function : Author
R. Buehler
  • Function : Author
S. Buson
  • Function : Author
G. A. Caliandro
  • Function : Author
R. A. Cameron
  • Function : Author
P. A. Caraveo
  • Function : Author
C. Cecchi
  • Function : Author
E. Charles
  • Function : Author
A. Chekhtman
  • Function : Author
S. Ciprini
  • Function : Author
R. Claus
  • Function : Author
S. Cutini
  • Function : Author
A. de Angelis
  • Function : Author
F. de Palma
  • Function : Author
C. D. Dermer
  • Function : Author
E. Do Couto E Silva
  • Function : Author
P. S. Drell
  • Function : Author
A. Drlica-Wagner
  • Function : Author
R. Dubois
  • Function : Author
C. Favuzzi
  • Function : Author
S. J. Fegan
E. C. Ferrara
  • Function : Author
W. B. Focke
  • Function : Author
M. Frailis
  • Function : Author
Y. Fukazawa
Y. Fukui
  • Function : Author
P. Fusco
  • Function : Author
F. Gargano
  • Function : Author
D. Gasparrini
  • Function : Author
S. Germani
  • Function : Author
N. Giglietto
P. Giommi
  • Function : Author
F. Giordano
  • Function : Author
M. Giroletti
  • Function : Author
T. Glanzman
  • Function : Author
G. Godfrey
  • Function : Author
J. E. Grove
  • Function : Author
S. Guiriec
  • Function : Author
D. Hadasch
Y. Hanabata
  • Function : Author
A. K. Harding
  • Function : Author
K. Hayashi
  • Function : Author
E. Hays
  • Function : Author
R. Itoh
  • Function : Author
G. Jóhannesson
  • Function : Author
A. S. Johnson
  • Function : Author
T. Kamae
  • Function : Author
H. Katagiri
  • Function : Author
J. Kataoka
  • Function : Author
H. Kubo
M. Kuss
  • Function : Author
J. Lande
  • Function : Author
L. Latronico
  • Function : Author
S.-H. Lee
  • Function : Author
A. M. Lionetto
  • Function : Author
F. Longo
F. Loparco
  • Function : Author
M. N. Lovellette
  • Function : Author
P. Lubrano
  • Function : Author
M. N. Mazziotta
  • Function : Author
P. F. Michelson
  • Function : Author
T. Mizuno
  • Function : Author
A. A. Moiseev
  • Function : Author
C. Monte
  • Function : Author
M. E. Monzani
  • Function : Author
A. Morselli
  • Function : Author
I. V. Moskalenko
  • Function : Author
S. Murgia
  • Function : Author
T. Nakamori
S. Nishino
  • Function : Author
P. L. Nolan
  • Function : Author
J. P. Norris
  • Function : Author
M. Ohno
  • Function : Author
T. Ohsugi
  • Function : Author
A. Okumura
  • Function : Author
N. Omodei
  • Function : Author
E. Orlando
  • Function : Author
J. F. Ormes
  • Function : Author
D. Paneque
D. Parent
  • Function : Author
M. Pesce-Rollins
T.A. Porter
  • Function : Author
S. Rainò
  • Function : Author
R. Rando
  • Function : Author
A. Reimer
O. Reimer
  • Function : Author
T. Reposeur
M. Roth
  • Function : Author
H. F.-W. Sadrozinski
  • Function : Author
C. Sgrò
  • Function : Author
E. J. Siskind
  • Function : Author
P. D. Smith
  • Function : Author
G. Spandre
  • Function : Author
P. Spinelli
  • Function : Author
D. J. Suson
  • Function : Author
H. Tajima
  • Function : Author
H. Takahashi
  • Function : Author
T. Tanaka
J. G. Thayer
  • Function : Author
J. B. Thayer
  • Function : Author
L. Tibaldo
  • Function : Author
O. Tibolla
  • Function : Author
D. F. Torres
  • Function : Author
G. Tosti
  • Function : Author
A. Tramacere
  • Function : Author
E. Troja
  • Function : Author
Y. Uchiyama
  • Function : Author
T. Uehara
  • Function : Author
T. L. Usher
  • Function : Author
J. Vandenbroucke
  • Function : Author
A. van Etten
  • Function : Author
G. Vianello
  • Function : Author
V. Vitale
A. P. Waite
  • Function : Author
P. Wang
  • Function : Author
B. L. Winer
  • Function : Author
K. S. Wood
  • Function : Author
H. Yamamoto
  • Function : Author
R. Yamazaki
  • Function : Author
Z. Yang
  • Function : Author
H. Yasuda
  • Function : Author
M. Ziegler
  • Function : Author
S. Zimmer
  • Function : Author

Abstract

We present a detailed analysis of the GeV gamma-ray emission toward the supernova remnant (SNR) G8.7-0.1 with the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope. An investigation of the relationship between G8.7-0.1 and the TeV unidentified source HESS J1804-216 provides us with an important clue on diffusion process of cosmic rays if particle acceleration operates in the SNR. The GeV gamma-ray emission is extended with most of the emission in positional coincidence with the SNR G8.7-0.1 and a lesser part located outside the western boundary of G8.7-0.1. The region of the gamma-ray emission overlaps spatially connected molecular clouds, implying a physical connection for the gamma-ray structure. The total gamma-ray spectrum measured with LAT from 200 MeV-100 GeV can be described by a broken power-law function with a break of 2.4 ± 0.6 (stat) ± 1.2 (sys) GeV, and photon indices of 2.10 ± 0.06 (stat) ± 0.10 (sys) below the break and 2.70 ± 0.12 (stat) ± 0.14 (sys) above the break. Given the spatial association among the gamma rays, the radio emission of G8.7-0.1, and the molecular clouds, the decay of π0s produced by particles accelerated in the SNR and hitting the molecular clouds naturally explains the GeV gamma-ray spectrum. We also find that the GeV morphology is not well represented by the TeV emission from HESS J1804-216 and that the spectrum in the GeV band is not consistent with the extrapolation of the TeV gamma-ray spectrum. The spectral index of the TeV emission is consistent with the particle spectral index predicted by a theory that assumes energy-dependent diffusion of particles accelerated in an SNR. We discuss the possibility that the TeV spectrum originates from the interaction of particles accelerated in G8.7-0.1 with molecular clouds, and we constrain the diffusion coefficient of the particles.

Dates and versions

in2p3-00664467 , version 1 (27-02-2012)

Identifiers

Cite

Marco Ajello, A. Allafort, Luca Baldini, Jean Ballet, Guido Barbiellini, et al.. FERMI LARGE AREA TELESCOPE OBSERVATIONS OF THE SUPERNOVA REMNANT G8.7-0.1. The Astrophysical Journal, 2012, 744, pp.80. ⟨10.1088/0004-637X/744/1/80⟩. ⟨in2p3-00664467⟩
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