A New Supernova Remnant Candidate and an Associated Outflow in the Sagittarius C Region

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dc.creatorTsuru, Takeshi Go
dc.creatorNobukawa, Masayoshi
dc.creatorNakajima, Hiroshi
dc.creatorMatsumoto, Hironori
dc.creatorKoyama, Katsuji
dc.creatorYamauchi, Shigeo
dc.date2009-02-08
dc.date.accessioned2026-07-07T12:39:22Z
dc.date.available2026-07-07T12:39:22Z
dc.descriptionWe present the Suzaku results on a new candidate of a supernova remnant (SNR) in the Sagittarius C region. We detected diffuse X-rays of an elliptical shape (G359.41-0.12) and a chimney-like structure (the Chimney), both of which were fitted with a thin thermal the model of kBT ~1 keV temperature. The absorption columns are same between these two structures, indicating that both are located at the same distance in the same line of sight. The narrow band image and one-dimensional profile of S XV Kalpha at 2.45 keV show that the Chimney is emanating from G359.41-0.12. Therefore, these two sources are physically connected with each other. The sum of the thermal energies of the Chimney and G359.41-0.12 is estimated to be 1.4x10^50 erg, typical for a galactic SNR. G359.41-0.12 is likely to be a new SNR candidate and the Chimney is an associated outflow.
dc.description10 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/0902.1308
dc.identifierhttp://arxiv.org/abs/0902.1308
dc.identifierPubl. Astron. Soc. Japan 61, S219-S223, 2009 January 30
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/219086
dc.subjectAstrophysics of Galaxies
dc.subjectHigh Energy Astrophysical Phenomena
dc.titleA New Supernova Remnant Candidate and an Associated Outflow in the Sagittarius C Region
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