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

doi:10.1051/0004-6361/201015131

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

Research output: Contribution to journal › Article › peer-review

24 Citations (Scopus)

Abstract

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€

Original language	English
Article number	L61
Journal	Astronomy and Astrophysics
Volume	521
Issue number	8
DOIs	https://doi.org/10.1051/0004-6361/201015131
Publication status	Published - 22-10-2010
Externally published	Yes

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1051/0004-6361/201015131

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title = "Origin of the dust emission from Tycho's SNR",

abstract = "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.{\^a}€",

author = "D. Ishihara and H. Kaneda and A. Furuzawa and H. Kunieda and T. Suzuki and Koo, \{B. C.\} and Lee, \{H. G.\} and Lee, \{J. J.\} and T. Onaka",

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doi = "10.1051/0004-6361/201015131",

language = "English",

volume = "521",

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TY - JOUR

T1 - Origin of the dust emission from Tycho's SNR

AU - Ishihara, D.

AU - Kaneda, H.

AU - Furuzawa, A.

AU - Kunieda, H.

AU - Suzuki, T.

AU - Koo, B. C.

AU - Lee, H. G.

AU - Lee, J. J.

AU - Onaka, T.

PY - 2010/10/22

Y1 - 2010/10/22

N2 - 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€

AB - 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€

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VL - 521

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 8

M1 - L61

ER -

Origin of the dust emission from Tycho's SNR

Abstract

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