Title: | Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946 |
Authors: | Acero, F. Aloisio, R. Amans, J. AMATO, Elena ANTONELLI, Lucio Angelo Aramo, C. Armstrong, T. Arqueros, F. Asano, K. Ashley, M. Backes, M. Fernández-Barral, A. Ferrand, G. Fesquet, M. Fiandrini, E. Fiasson, A. Filipović, M. D. FIORETTI, VALENTINA Font, L. Fontaine, G. Franco, F. J. Balazs, C. Freixas Coromina, L. Fujita, Y. Fukui, Y. Funk, S. Förster, A. Gadola, A. Garcia López, R. Garczarczyk, M. Giglietto, N. Giordano, F. Balzer, A. GIULIANI, ANDREA Glicenstein, J. Gnatyk, R. Goldoni, P. Grabarczyk, T. Graciani, R. Graham, J. GRANDI, PAOLA Granot, J. Green, A. J. Bamba, A. Griffiths, S. Gunji, S. Hakobyan, H. Hara, S. Hassan, T. Hayashida, M. Heller, M. Helo, J. C. Hinton, J. Hnatyk, B. Barkov, M. Huet, J. Huetten, M. Humensky, T. B. Hussein, M. Hörandel, J. Ikeno, Y. Inada, T. Inome, Y. Inoue, S. Inoue, T. Barrio, J. A. Inoue, Y. Ioka, K. Iori, M. Jacquemier, J. Janecek, P. Jankowsky, D. Jung, I. Kaaret, P. Katagiri, H. Kimeswenger, S. Benbow, W. Kimura, S. Knödlseder, J. Koch, B. Kocot, J. Kohri, K. Komin, N. Konno, Y. Kosack, K. Koyama, S. Kraus, M. Bernlöhr, K. Kubo, H. Kukec Mezek, G. Kushida, J. LA PALOMBARA, NICOLA Lalik, K. Lamanna, G. Landt, H. Lapington, J. Laporte, P. Lee, S. Beshley, V. Lees, J. Lefaucheur, J. Lenain, J. -P. LETO, Giuseppe Lindfors, E. Lohse, T. LOMBARDI, Saverio Longo, F. Lopez, M. LUCARELLI, Fabrizio BIGONGIARI, Ciro Luque-Escamilla, P. L. López-Coto, R. MACCARONE, MARIA CONCETTA Maier, G. MALAGUTI, GIUSEPPE Mandat, D. Maneva, G. Mangano, S. Marcowith, A. Martí, J. Biland, A. Martínez, M. Martínez, G. Masuda, S. Maurin, G. Maxted, N. Melioli, C. MINEO, TERESA Mirabal, N. Mizuno, T. Moderski, R. Bilinsky, A. Mohammed, M. Montaruli, T. Moralejo, A. Mori, K. MORLINO, GIOVANNI Morselli, A. Moulin, E. Mukherjee, R. Mundell, C. Muraishi, H. Bissaldi, E. Murase, K. Nagataki, S. Nagayoshi, T. Naito, T. Nakajima, D. Nakamori, T. Nemmen, R. Niemiec, J. Nieto, D. Nievas-Rosillo, M. Biteau, J. Nikołajuk, M. Nishijima, K. Noda, K. Nogues, L. Nosek, D. Novosyadlyj, B. Nozaki, S. Ohira, Y. Ohishi, M. Ohm, S. Blanch, O. Okumura, A. Ong, R. A. Orito, R. ORLATI, ANDREA Ostrowski, M. Oya, I. Padovani, Marco Palacio, J. Palatka, M. Paredes, J. M. Blasi, P. Pavy, S. Pe'er, A. PERSIC, Massimo Petrucci, P. Petruk, O. Pisarski, A. Pohl, M. Porcelli, A. PRANDINI, ELISA Prast, J. Blazek, J. PRINCIPE, GIACOMO Prouza, M. Pueschel, E. Pühlhofer, G. Quirrenbach, A. Rameez, M. Reimer, O. Renaud, M. Ribó, M. Rico, J. Boisson, C. Rizi, V. Rodriguez, J. Rodriguez Fernandez, G. Rodríguez Vázquez, J. J. ROMANO, Patrizia ROMEO, Giuseppe Rosado, J. Rousselle, J. Rowell, G. Rudak, B. BONANNO, Giovanni Sadeh, I. Safi-Harb, S. Saito, T. Sakaki, N. Sanchez, D. SANGIORGI, Pierluca Sano, H. Santander, M. Sarkar, S. Sawada, M. Bonardi, A. Schioppa, E. J. Schoorlemmer, H. Schovanek, P. Schussler, F. Sergijenko, O. Servillat, M. Shalchi, A. Shellard, R. C. Siejkowski, H. Sillanpää, A. Bonavolontà, C. Simone, D. Sliusar, V. Sol, H. Stanič, S. Starling, R. Stawarz, Ł. Stefanik, S. Stephan, M. Stolarczyk, T. Szanecki, M. Bonnoli, G. Szepieniec, T. TAGLIAFERRI, Gianpiero Tajima, H. Takahashi, M. Takeda, J. Tanaka, M. Tanaka, S. Tejedor, L. A. Telezhinsky, I. Temnikov, P. Braiding, C. Terada, Y. Tescaro, D. Teshima, M. TESTA, Vincenzo Thoudam, S. Tokanai, F. Torres, D. F. TORRESI, ELEONORA Tosti, G. Townsley, C. Brau-Nogué, S. Travnicek, P. Trichard, C. TRIFOGLIO, MASSIMO Tsujimoto, S. Vagelli, V. VALLANIA, PIERO Valore, L. van Driel, W. van Eldik, C. Vandenbroucke, J. Bregeon, J. Vassiliev, V. Vecchi, M. VERCELLONE, STEFANO Vergani, S. Vigorito, C. Vorobiov, S. Vrastil, M. Vázquez Acosta, M. L. Wagner, S. J. Wagner, R. Brown, A. M. Wakely, S. P. Walter, R. Ward, J. E. Watson, J. J. Weinstein, A. White, M. White, R. Wierzcholska, A. Wilcox, P. Williams, D. A. Bugaev, V. Wischnewski, R. Wojcik, P. Yamamoto, T. Yamamoto, H. Yamazaki, R. Yanagita, S. Yang, L. Yoshida, T. Yoshida, M. Yoshiike, S. BULGARELLI, ANDREA Yoshikoshi, T. Zacharias, M. ZAMPIERI, Luca Zanin, R. Zavrtanik, M. Zavrtanik, D. Zdziarski, A. Zech, A. Zechlin, H. Zhdanov, V. Bulik, T. Ziegler, A. Zorn, J. Burton, M. Burtovoi, A. Busetto, G. Böttcher, M. Cameron, R. CAPALBI, Milvia Caproni, A. CARAVEO, PATRIZIA Carosi, R. CASCONE, Enrico Cerruti, M. Chaty, S. Chen, A. Chen, X. Chernyakova, M. Chikawa, M. Chudoba, J. Cohen-Tanugi, J. Colafrancesco, S. CONFORTI, Vito Contreras, J. L. COSTA, Alessandro Cotter, G. COVINO, Stefano Covone, G. Cumani, P. CUSUMANO, GIANCARLO D'AMMANDO, FILIPPO D'Urso, D. Daniel, M. Dazzi, F. De Angelis, A. DE CESARE, GIOVANNI De Franco, A. De Frondat, F. de Gouveia Dal Pino, E. M. De Lisio, C. de los Reyes Lopez, R. De Lotto, B. de Naurois, M. De Palma, F. DEL SANTO, MELANIA Delgado, C. della Volpe, D. Di Girolamo, T. Di Giulio, C. Di Pierro, F. Di Venere, L. Doro, M. Dournaux, J. Dumas, D. Dwarkadas, V. Díaz, C. Ebr, J. Egberts, K. Einecke, S. Elsässer, D. Eschbach, S. Falceta-Goncalves, D. Fasola, G. Fedorova, E. |
Issue Date: | 2017 |
Journal: | THE ASTROPHYSICAL JOURNAL |
Number: | 840 |
Issue: | 2 |
First Page: | 74 |
Abstract: | We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX J1713.7-3946, a young supernova remnant (SNR) and one of the brightest sources ever discovered in very high energy (VHE) gamma rays. Special attention is paid to exploring possible spatial (anti)correlations of gamma rays with emission at other wavelengths, in particular X-rays and CO/H I emission. We present a series of simulated images of RX J1713.7-3946 for CTA based on a set of observationally motivated models for the gamma-ray emission. In these models, VHE gamma rays produced by high-energy electrons are assumed to trace the nonthermal X-ray emission observed by XMM-Newton, whereas those originating from relativistic protons delineate the local gas distributions. The local atomic and molecular gas distributions are deduced by the NANTEN team from CO and H I observations. Our primary goal is to show how one can distinguish the emission mechanism(s) of the gamma rays (I.e., hadronic versus leptonic, or a mixture of the two) through information provided by their spatial distribution, spectra, and time variation. This work is the first attempt to quantitatively evaluate the capabilities of CTA to achieve various proposed scientific goals by observing this important cosmic particle accelerator. |
URI: | http://hdl.handle.net/20.500.12386/26912 |
URL: | https://iopscience.iop.org/article/10.3847/1538-4357/aa6d67 |
ISSN: | 0004-637X |
DOI: | 10.3847/1538-4357/aa6d67 |
Bibcode ADS: | 2017ApJ...840...74A |
Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista
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