File:IRAS 00500+6713.jpg
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Captions
Captions
A comparison between an observed image (left panel; X-ray image (XMM) and IR contours (WISE)) and schematic picture of IRAS 00500+671
Summary
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| Description |
English: A comparison between an observed image (left panel; X-ray image (XMM) and IR contours (WISE)) and schematic picture of IRAS 00500+6713 (right panel). The schematic picture includes the morphology of IRAS 00500+6713 inferred from multiwavelength observations (the left semicircle) and our dynamical model (the right semicircle). A dusty IR ring is sandwiched by the inner and outer X-ray nebulae. We assume that the inner X-ray nebula corresponds to the wind termination shock while the outer X-ray nebula to the shocked interface between the ejecta of SN 1181 and the ISM, and the dust ring corresponds to the unshocked SN ejecta. |
| Date | |
| Source | A Dynamical Model for IRAS 00500+6713: The Remnant of a Type Iax Supernova SN 1181 Hosting a Double Degenerate Merger Product WD J005311 - 2024 July 5, IOPscience, American Astronomical Society, Astrophysical Journal, Volume 969, Number 2 (Takatoshi Ko et al 2024 ApJ 969 116) |
| Author | Takatoshi Ko, Hiromasa Suzuki, Kazumi Kashiyama, Hiroyuki Uchida, Takaaki Tanaka, Daichi Tsuna, Kotaro Fujisawa, Aya Bamba, and Toshikazu Shigeyama |
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This file is licensed under the Creative Commons Attribution 4.0 International license.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 12:29, 5 July 2024 | | 2,031 × 906 (608 KB) | Artem.G (talk | contribs) | Uploaded a work by Takatoshi Ko et al from https://iopscience.iop.org/article/10.3847/1538-4357/ with UploadWizard |
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