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  5. Deeper H.E.S.S. observations of Vela Junior (RX J0852.0-4622): Morphology studies and resolved spectroscopy
 

Deeper H.E.S.S. observations of Vela Junior (RX J0852.0-4622): Morphology studies and resolved spectroscopy

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2018
Author(s)
H. E. S. S. Collaboration
•
Abdalla, H.
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Abramowski, A.
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Aharonian, F.
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Ait Benkhali, F.
•
Akhperjanian, A. G.
•
Angüner, E. O.
•
Arakawa, M.
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Arrieta, M.
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Aubert, P.
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Backes, M.
•
Balzer, A.
•
Barnard, M.
•
Becherini, Y.
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Becker Tjus, J.
•
Berge, D.
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Bernhard, S.
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Bernlöhr, K.
•
Blackwell, R.
•
Böttcher, M.
•
Boisson, C.
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Bolmont, J.
•
Bordas, P.
•
Bregeon, J.
•
Brun, F.
•
Brun, P.
•
Bryan, M.
•
Büchele, M.
•
Bulik, T.
•
Capasso, M.
•
Carr, J.
•
Casanova, S.
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Cerruti, M.
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Chakraborty, N.
•
Chalme-Calvet, R.
•
Chaves, R. C. G.
•
Chen, A.
•
Chevalier, J.
•
Chrétien, M.
•
Coffaro, M.
•
Colafrancesco, S.
•
Cologna, G.
•
Condon, B.
•
Conrad, J.
•
Cui, Y.
•
Davids, I. D.
•
Decock, J.
•
Degrange, B.
•
Deil, C.
•
Devin, J.
•
deWilt, P.
•
Dirson, L.
•
Djannati-Ataï, A.
•
Domainko, W.
•
Donath, A.
•
Drury, L. O. 'C.
•
Dutson, K.
•
Dyks, J.
•
Edwards, T.
•
Egberts, K.
•
Eger, P.
•
Ernenwein, J. -P.
•
Eschbach, S.
•
Farnier, C.
•
Fegan, S.
•
Fernandes, M. V.
•
Fiasson, A.
•
Fontaine, G.
•
Förster, A.
•
Funk, S.
•
Füßling, M.
•
Gabici, S.
•
Gajdus, M.
•
Gallant, Y. A.
•
Garrigoux, T.
•
Giavitto, G.
•
Giebels, B.
•
Glicenstein, J. F.
•
Gottschall, D.
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Goyal, A.
•
Grondin, M. -H.
•
Hahn, J.
•
Haupt, M.
•
Hawkes, J.
•
Heinzelmann, G.
•
Henri, G.
•
Hermann, G.
•
Hervet, O.
•
Hinton, J. A.
•
Hofmann, W.
•
Hoischen, C.
•
Holler, M.
•
Horns, D.
•
Ivascenko, A.
•
Iwasaki, H.
•
Jacholkowska, A.
•
Jamrozy, M.
•
Janiak, M.
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Jankowsky, D.
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Jankowsky, F.
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Jingo, M.
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Jogler, T.
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Jouvin, L.
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Jung-Richardt, I.
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Kastendieck, M. A.
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Katarzyński, K.
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Katsuragawa, M.
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Katz, U.
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Kerszberg, D.
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Khangulyan, D.
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Khélifi, B.
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Kieffer, M.
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King, J.
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Klepser, S.
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Klochkov, D.
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Kluźniak, W.
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Kolitzus, D.
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Komin, Nu.
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Krakau, S.
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Kraus, M.
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Krüger, P. P.
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Laffon, H.
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Lamanna, G.
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Lau, J.
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Lees, J. -P.
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Lefaucheur, J.
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Lefranc, V.
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Lemière, A.
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Lemoine-Goumard, M.
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Lenain, J. -P.
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Leser, E.
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Lohse, T.
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Lorentz, M.
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Liu, R.
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López-Coto, R.
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Lypova, I.
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Marandon, V.
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Marcowith, A.
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Mariaud, C.
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Marx, R.
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Maurin, G.
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Maxted, N.
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Mayer, M.
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Meintjes, P. J.
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Meyer, M.
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Mitchell, A. M. W.
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Moderski, R.
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Mohamed, M.
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Mohrmann, L.
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Morå, K.
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Moulin, E.
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Murach, T.
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Nakashima, S.
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de Naurois, M.
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Niederwanger, F.
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Niemiec, J.
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Oakes, L.
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O'Brien, P.
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Odaka, H.
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Öttl, S.
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Ohm, S.
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Ostrowski, M.
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Oya, I.
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Padovani, Marco  
•
Panter, M.
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Parsons, R. D.
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Paz Arribas, M.
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Pekeur, N. W.
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Pelletier, G.
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Perennes, C.
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Petrucci, P. -O.
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Peyaud, B.
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Piel, Q.
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Pita, S.
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Poon, H.
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Prokhorov, D.
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Prokoph, H.
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Pühlhofer, G.
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Punch, M.
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Quirrenbach, A.
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Raab, S.
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Reimer, A.
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Reimer, O.
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Renaud, M.
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de los Reyes, R.
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Richter, S.
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Rieger, F.
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Romoli, C.
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Rowell, G.
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Rudak, B.
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Rulten, C. B.
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Sahakian, V.
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Saito, S.
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Salek, D.
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Sanchez, D. A.
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Santangelo, A.
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Sasaki, M.
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Schlickeiser, R.
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Schüssler, F.
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Schulz, A.
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Schwanke, U.
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Schwemmer, S.
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Seglar-Arroyo, M.
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Settimo, M.
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Seyffert, A. S.
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Shafi, N.
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Shilon, I.
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Simoni, R.
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Sol, H.
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Spanier, F.
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Spengler, G.
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Spies, F.
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Stawarz, Ł.
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Steenkamp, R.
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Stegmann, C.
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Stycz, K.
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Sushch, I.
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Takahashi, T.
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Tavernet, J. -P.
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Tavernier, T.
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Taylor, A. M.
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Terrier, R.
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Tibaldo, L.
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Tiziani, D.
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Tluczykont, M.
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Trichard, C.
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Tsuji, N.
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Tuffs, R.
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Uchiyama, Y.
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van der Walt, D. J.
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van Eldik, C.
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van Rensburg, C.
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van Soelen, B.
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Vasileiadis, G.
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Veh, J.
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Venter, C.
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Viana, A.
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Vincent, P.
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Vink, J.
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Voisin, F.
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Völk, H. J.
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Vuillaume, T.
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Wadiasingh, Z.
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Wagner, S. J.
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Wagner, P.
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Wagner, R. M.
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White, R.
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Wierzcholska, A.
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Willmann, P.
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Wörnlein, A.
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Wouters, D.
•
Yang, R.
•
Zabalza, V.
•
Zaborov, D.
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Zacharias, M.
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Zanin, R.
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Zdziarski, A. A.
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Zech, A.
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Zefi, F.
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Ziegler, A.
•
Żywucka, N.
DOI
10.1051/0004-6361/201630002
Abstract

Aims: We study γ-ray emission from the shell-type supernova remnant (SNR) RX J0852.0-4622 to better characterize its spectral properties and its distribution over the SNR.
Methods: The analysis of an extended High Energy Spectroscopic System (H.E.S.S.) data set at very high energies (E > 100 GeV) permits detailed studies, as well as spatially resolved spectroscopy, of the morphology and spectrum of the whole RX J0852.0-4622 region. The H.E.S.S. data are combined with archival data from other wavebands and interpreted in the framework of leptonic and hadronic models. The joint Fermi-LAT-H.E.S.S. spectrum allows the direct determination of the spectral characteristics of the parent particle population in leptonic and hadronic scenarios using only GeV-TeV data.
Results: An updated analysis of the H.E.S.S. data shows that the spectrum of the entire SNR connects smoothly to the high-energy spectrum measured by Fermi-LAT. The increased data set makes it possible to demonstrate that the H.E.S.S. spectrum deviates significantly from a power law and is well described by both a curved power law and a power law with an exponential cutoff at an energy of Ecut = (6.7 ± 1.2stat ± 1.2syst) TeV. The joint Fermi-LAT-H.E.S.S. spectrum allows the unambiguous identification of the spectral shape as a power law with an exponential cutoff. No significant evidence is found for a variation of the spectral parameters across the SNR, suggesting similar conditions of particle acceleration across the remnant. A simple modeling using one particle population to model the SNR emission demonstrates that both leptonic and hadronic emission scenarios remain plausible. It is also shown that at least a part of the shell emission is likely due to the presence of a pulsar wind nebula around PSR J0855-4644.

A FITS image of the region of interest and two text files describing the H.E.S.S. spectrum of RX J0852.0-4622 are only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/612/A7

Volume
612
Start page
A7
Uri
http://hdl.handle.net/20.500.12386/27717
Url
https://www.aanda.org/articles/aa/abs/2018/09/aa33202-18/aa33202-18.html
Issn Identifier
0004-6361
Ads BibCode
2018A&A...612A...7H
Rights
open.access
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