1. First Detection of Ar-K Line Emission from the Cygnus Loop
- Author
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Hiroshi Tsunemi, Hiroyuki Uchida, Hiroko Kosugi, Satoru Katsuda, Hiroaki Takahashi, S. Takakura, Nozomu Tominaga, and Masashi Kimura
- Subjects
Physics ,Cygnus Loop ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics ,EPIC ,K-line ,Spectral line ,Astrophysics - Solar and Stellar Astrophysics ,Space and Planetary Science ,Emission spectrum ,Ejecta ,Supernova remnant ,Solar and Stellar Astrophysics (astro-ph.SR) ,Line (formation) - Abstract
We observed the Cygnus Loop with XMM-Newton (9 pointings) and Suzaku (32 pointings) between 2002 and 2008. The total effective exposure time is 670.2 ks. By using all of the available data, we intended to improve a signal-to-noise ratio of the spectrum. Accordingly, the accumulated spectra obtained by the XIS and the EPIC show some line features around 3 keV that are attributed to the S He$\beta$ and Ar He$\alpha$ lines, respectively. Since the Cygnus Loop is an evolved ($\sim$10,000 yr) supernova remnant whose temperature is relatively low ($, Comment: 12 pages, 9 figures, accepted for publication in PASJ
- Published
- 2011
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