SIMBAD references

2017ApJ...842...22E - Astrophys. J., 842, 22-22 (2017/June-2)

Recombining plasma and gamma-ray emission in the mixed-morphology supernova remnant 3C 400.2.

ERGIN T., SEZER A., SANO H., YAMAZAKI R. and FUKUI Y.

Abstract (from CDS):

3C 400.2 belongs to the mixed-morphology supernova remnant class, showing center-filled X-ray and shell-like radio morphology. We present a study of 3C 400.2 with archival Suzaku and Fermi-LAT observations. We find recombining plasma (RP) in the Suzaku spectra of north-east and south-east regions. The spectra of these regions are well described by two-component thermal plasma models: the hard component is in RP, while the soft component is in collisional ionization equilibrium (CIE) conditions. The RP has enhanced abundances, indicating that the X-ray emission has an ejecta origin, while the CIE has solar abundances associated with the interstellar material. The X-ray spectra of north-west and south-west regions are best fitted by a two-component thermal plasma model: an ionizing and a CIE plasma. We have detected GeV gamma-ray emission from 3C 400.2 at the level of ∼5σ, assuming a point-like source model with a power-law (PL) type spectrum. We have also detected a new GeV source at the level of ∼13σ, assuming a Gaussian extension model with a PL-type spectrum in the neighborhood of the supernova remnant. We report the analysis results of 3C 400.2 and the new extended gamma-ray source, and discuss the nature of gamma-ray emission of 3C 400.2 in the context of existing NANTEN CO data, Dominion Radio Astrophysical Observatory H I data, and the Suzaku X-ray analysis results.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): gamma-rays: ISM - ISM: clouds - ISM: individual objects: G53.6-2.2, 3C 400.2 - ISM: supernova remnants - X-rays: ISM - X-rays: ISM

Nomenclature: [ESS2017] PS JHHMM.m+DDMM (Nos PS J1934.5+1845, PS J1938.6+1722).

Simbad objects: 13

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2020.09.30-23:37:43

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