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https://hdl.handle.net/2440/119832
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dc.contributor.author | Sano, H. | - |
dc.contributor.author | Rowell, G. | - |
dc.contributor.author | Reynoso, E.M. | - |
dc.contributor.author | Jung-Richardt, I. | - |
dc.contributor.author | Yamane, Y. | - |
dc.contributor.author | Nagaya, T. | - |
dc.contributor.author | Yoshiike, S. | - |
dc.contributor.author | Hayashi, K. | - |
dc.contributor.author | Torii, K. | - |
dc.contributor.author | Maxted, N. | - |
dc.contributor.author | Mitsuishi, I. | - |
dc.contributor.author | Inoue, T. | - |
dc.contributor.author | Inutsuka, S. | - |
dc.contributor.author | Yamamoto, H. | - |
dc.contributor.author | Tachihara, K. | - |
dc.contributor.author | Fukui, Y. | - |
dc.date.issued | 2019 | - |
dc.identifier.citation | The Astrophysical Journal: an international review of astronomy and astronomical physics, 2019; 876(1):37-1-37-13 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.issn | 1538-4357 | - |
dc.identifier.uri | http://hdl.handle.net/2440/119832 | - |
dc.description.abstract | We present a detailed morphological study of TeV gamma-rays, synchrotron radiation, and interstellar gas in the young Type Ia supernova remnant (SNR) RCW 86. We find that the interstellar atomic gas shows good spatial correlation with the gamma-rays, indicating that the TeV gamma-rays from RCW 86 are likely predominantly of hadronic origin. In contrast, the spatial correlation between the interstellar molecular cloud and the TeV gamma-rays is poor in the southeastern shell of the SNR. We argue that this poor correlation can be attributed to the low-energy cosmic rays (~1 TeV) not penetrating into the dense molecular cloud due to an enhancement of the turbulent magnetic field around the dense cloud of ~10–100 μG. We also find that the southwestern shell, which is bright in both synchrotron X-ray and radio continuum radiation, shows a significant gamma-ray excess compared with the interstellar proton column density, suggesting that leptonic gamma-rays via inverse Compton scattering possibly contribute alongside the hadronic gamma-rays. The total cosmic-ray energies of the young TeV gamma-ray SNRs—RX J1713.7−3946, Vela Jr, HESS J1731−347, and RCW 86—are roughly similar, which indicates that cosmic rays can be accelerated in both the core-collapse and Type Ia supernovae. The total energy of cosmic rays derived using the gas density, ~10⁴⁸–10⁴⁹ erg, gives a safe lower limit due mainly to the low filling factor of interstellar gas within the shell. | - |
dc.description.statementofresponsibility | H. Sano, G. Rowell, E.M. Reynoso, I. Jung-Richardt, Y. Yamane, T. Nagaya, S. Yoshiike, K. Hayashi, K. Torii, N. Maxted, I. Mitsuishi, T. Inoue, S. Inutsuka, H. Yamamoto, K. Tachihara, and Y. Fukui | - |
dc.language.iso | en | - |
dc.publisher | American Astronomical Society; IOP Publishing | - |
dc.rights | © 2019. The American Astronomical Society. All rights reserved. | - |
dc.source.uri | http://dx.doi.org/10.3847/1538-4357/ab108f | - |
dc.subject | Cosmic rays; gamma rays: ISM; ISM: clouds; ISM: individual objects (RCW 86); ISM: supernova remnants | - |
dc.title | Possible evidence for cosmic-ray acceleration in the Type Ia SNR RCW 86: spatial correlation between TeV gamma-rays and interstellar atomic protons | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.3847/1538-4357/ab108f | - |
dc.relation.grant | ARC | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Rowell, G. [0000-0002-9516-1581] | - |
Appears in Collections: | Aurora harvest 4 Physics publications |
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