Overionized plasma in the supernova remnant Sagittarius A East anchored by XRISM observations
Collaboration
9 pages
Published in:
- Publ.Astron.Soc.Jap. 77 (2025) 1, L1-L8
- Published: Dec 26, 2024
e-Print:
- 2412.00676 [astro-ph.HE]
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Abstract: (Oxford University Press)
Sagittarius A East is a supernova remnant with a unique surrounding environment, as it is located in the immediate vicinity of the supermassive black hole at the Galactic center, Sagittarius A∗. The X-ray emission of the remnant is suspected to show features of overionized plasma, which would require peculiar evolutionary paths. We report on the first observation of Sagittarius A East with the X-Ray Imaging and Spectroscopy Mission (XRISM). Equipped with a combination of a high-resolution microcalorimeter spectrometer and a large field-of-view CCD imager, we for the first time resolved the Fe xxv K-shell lines into fine structure lines and measured the forbidden-to-resonance intensity ratio to be 1.39±0.12, which strongly suggests the presence of overionized plasma. We obtained a reliable constraint on the ionization temperature just before the transition into the overionization state, of >4keV. The recombination timescale was constrained to be <8×1011cm−3s. The small velocity dispersion of 109±6kms−1 indicates a low Fe ion temperature <8keV and a small expansion velocity <200kms−1. The high initial ionization temperature and small recombination timescale suggest that either rapid cooling of the plasma via adiabatic expansion from dense circumstellar material or intense photoionization by Sagittarius A∗ in the past may have triggered the overionization.Note:
- 9 pages, 4 figures, accepted for publication in PASJ. Corresponding authors: Hiromasa Suzuki, Hideki Uchiyama, Masayoshi Nobukawa, and Yuki Amano
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