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2023PASJ...75..907F - Publ. Astron. Soc. Jap., 75, 907-912 (2023/October-0)
Suzaku spectral analysis of an X-ray emitting plasma in the supernova remnant G352.7-0.1.
FUJISHIGE A., YAMAUCHI S., NOBUKAWA K.K. and NOBUKAWA M.
Abstract (from CDS):
The results of a Suzaku observation of the supernova remnant (SNR) G352.7-0.1 are presented in this paper. We conducted spectral analysis based on careful sky background estimation and found an emission line from Al at 1.6 keV, in addition to previously detected emission lines from Mg, Si, S, Ar, Ca, and Fe ions. The X-ray spectrum in the 0.7-10 keV band is represented by a two-component ionizing plasma model with different temperatures and ionization timescales. Based on the results, properties of the X-ray emitting plasma and the explosion type are discussed.
Abstract Copyright: © The Author(s) 2023. Published by Oxford University Press on behalf of the Astronomical Society of Japan.
Journal keyword(s): ISM: individual objects (G352.7-0.1) - ISM: supernova remnants - X-rays: ISM
Simbad objects: 8
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