Progenitor Constraint-incorporating Shell Merger: The Case of Supernova Remnant G359.0–0.9
- DOI
- 10.3847/1538-4357/ad5284
- Published
- 2024-07-01
- Container
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Open access
- unknown
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Cite this work
BibTeX
@article{allodium:10.3847/1538-4357/ad5284,
title = {Progenitor Constraint-incorporating Shell Merger: The Case of Supernova Remnant G359.0–0.9},
author = {Kai Matsunaga and Hiroyuki Uchida and Rei Enokiya and Toshiki Sato and Ryo Sawada and Hideyuki Umeda and Takuto Narita and Takeshi Go Tsuru},
year = {2024},
journal = {The Astrophysical Journal},
doi = {10.3847/1538-4357/ad5284},
url = {https://doi.org/10.3847/1538-4357/ad5284}
}RIS
TY - JOUR TI - Progenitor Constraint-incorporating Shell Merger: The Case of Supernova Remnant G359.0–0.9 AU - Kai Matsunaga AU - Hiroyuki Uchida AU - Rei Enokiya AU - Toshiki Sato AU - Ryo Sawada AU - Hideyuki Umeda AU - Takuto Narita AU - Takeshi Go Tsuru PY - 2024 JO - The Astrophysical Journal DO - 10.3847/1538-4357/ad5284 UR - https://doi.org/10.3847/1538-4357/ad5284 ER -
APA
Matsunaga, K., Uchida, H., Enokiya, R., Sato, T., Sawada, R., Umeda, H., Narita, T., & Tsuru, T. G. (2024). Progenitor Constraint-incorporating Shell Merger: The Case of Supernova Remnant G359.0–0.9. The Astrophysical Journal. https://doi.org/10.3847/1538-4357/ad5284
Source records
- crossref · retrieved 2026-09-25T10:07:00.743Z