Origin of the dust emission from Tycho's SNR

D. Ishihara, H. Kaneda, A. Furuzawa, H. Kunieda, T. Suzuki, B. C. Koo, H. G. Lee, J. J. Lee, T. Onaka

研究成果: Article査読

22 被引用数 (Scopus)

抄録

Aims. We investigate the spatial distribution of dust emission around Tycho's SNR to understand its origin. We distinguish the dust associated with the SNR from that of the surrounding ISM. Methods. We performed mid- to far-infrared imaging observations of the remnant at wavelengths of 9, 15, 18, 24, 65, 90, 140, and 160 μm using the Infrared Camera and the Far-Infrared Surveyor onboard AKARI. We compared the AKARI images with the Suzaku X-ray image and the 12CO image of Tycho's SNR. Results. All the AKARI images except the 9, 140, and 160 μm band images show a shell-like emission structure with brightness peaks at the northeast (NE) and northwest (NW) boundaries, sharply outlining part of the X-ray shell.â€

本文言語English
論文番号L61
ジャーナルAstronomy and Astrophysics
521
8
DOI
出版ステータスPublished - 22-10-2010

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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