Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011pasj...63s.837y&link_type=abstract
Publications of the Astronomical Society of Japan, Vol.63, No.SP3, pp.S837-S848
Astronomy and Astrophysics
Astronomy
1
Ism: Individual (Rcw 86), Supernova Remnants, X-Rays: Spectra
Scientific paper
We report on results of imaging and spectral analysis of the supernova remnant (SNR) RCW 86 observed with Suzaku. The SNR is known to exhibit K-shell emission of low ionized Fe, possibly originating from supernova ejecta. We revealed the global distribution of the Fe-rich plasma in the entire remnant, for the first time; the Fe-K emission was clearly detected from the west, north, and south regions, in addition to the X-ray brighter shells of southwest and northeast, where the presence of the Fe-rich ejecta has already been reported. The spectrum of each region is well represented by a three-component model consisting of low- and high-temperature thermal plasmas and non-thermal emission. The lower-temperature component, with elemental abundances of near the solar values, likely originates from the forward shocked interstellar medium, while the Fe-rich ejecta is described by the hotter plasma. From the morphologies of the forward and reverse shocks in the west region, the total ejecta mass is estimated to be 1-2Modot for the typical explosion energy of ˜1 × 1051 erg. The integrated flux of the Fe-K emission from the entire SNR roughly corresponds to a total Fe mass of about 1Modot. Both of these estimates suggest a Type Ia supernova origin of this SNR. We also find possible evidence of an Fe-rich clump located beyond the forward-shock front in the north rim, which is reminiscent of ejecta knots observed in the Tycho and Vela SNRs.
Koyama Katsuji
Uchida Hiroyuki
Yamaguchi Hiroya
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