Optical reconstruction of dust in the region of supernova remnant RX J1713.7−3946 from astrometric data
Author:
Funder
NOVA | Faculdade de Ciências e Tecnologia, Universidade Nova de Lisboa
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-021-01344-w.pdf
Reference43 articles.
1. Aharonian, F. A. Gamma rays from supernova remnants. Astropart. Phys. 43, 71–80 (2013).
2. Aharonian, F., Ruizhi, Y. & de Oña Wilhelmi, E. Massive stars as major factories of Galactic cosmic rays. Nat. Astron. 3, 561–567 (2019).
3. Abdalla, H. et al. H.E.S.S. observations of RX J1713.7−3946 with improved angular and spectral resolution: evidence for gamma-ray emission extending beyond the X-ray emitting shell. Astron. Astrophys. 612, A6 (2018).
4. Slane, P. et al. Non-thermal X-ray emission from the shell-type supernova remnant G347.3−0.5. Astrophys. J. 525, 357 (1999).
5. Sano, H. et al. A detailed study of non-thermal X-ray properties and Interstellar gas toward the γ-ray supernova remnant RX J1713.7−3946. Astrophys. J. 729, 175 (2015).
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