Figure 3 from ALMA CO Observations of the Gamma-Ray Supernova Remnant RX J1713.7–3946: Discovery of Shocked Molecular Cloudlets and Filaments at 0.01 pc Scales

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ALMA CO Observations of the Gamma-Ray Supernova Remnant RX J1713.7–3946: Discovery of Shocked Molecular Cloudlets and Filaments at 0.01 pc Scales

Authors: H. Sano, T. Inoue, K. Tokuda, T. Tanaka, R. Yamazaki, S. Inutsuka, F. Aharonian, G. Rowell, M. D. Filipović, Y. Yamane, S. Yoshiike, N. Maxted, H. Uchida, T. Hayakawa, K. Tachihara, Y. Uchiyama, and Y. Fukui

2020 The Astrophysical Journal Letters 904 L24.

Provider: AAS Journals

Caption: Figure 3.

(a) Enlarged view of ALMA CO map toward an X-ray hotspot presented by Uchiyama et al. (2007). (b–h) Sequence of X-ray observations in 2000 July, 2005 July, 2006 May, 2009 January, 2009 May, 2009 September, and 2011 July. All X-ray images show the same intensity scales. Superposed contours indicate the CO intensity. Gray shaded areas were eliminated due to low exposure time (see the text).

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