Probing the nova shock physics with future gamma-ray observations of the upcoming outburst from T Coronae Borealis-Reference-Cited by-同舟云学术

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Probing the nova shock physics with future gamma-ray observations of the upcoming outburst from T Coronae Borealis

Published:2024-08 Issue: Volume:43 Page:171-177
ISSN:2214-4048
Container-title:Journal of High Energy Astrophysics
language:en
Short-container-title:Journal of High Energy Astrophysics

Author:

Zheng Jian-He^ORCID,Zhang Hai-Ming,Liu Ruo-Yu,Zha Min,Wang Xiang-Yu

Funder

NSFC

Publisher

Elsevier BV

Reference52 articles.

1. Estimating distances from parallaxes. V. Geometric and photogeometric distances to 1.47 billion stars in Gaia early data release 3;Bailer-Jones;Astron. J.,2021

2. New binary parameters for the symbiotic recurrent nova T Coronae Borealis;Belczynski;Mon. Not. R. Astron. Soc.,1998

3. Spectroscopic orbits and variations of RS Ophiuchi;Brandi;Astron. & Astrophys.,2009

4. On the escape of particles from cosmic ray modified shocks;Caprioli;Mon. Not. R. Astron. Soc.,2009

5. Comprehensive models of novae at metallicity Z = 0.02 and Z = 10−4;Chen;Mon. Not. R. Astron. Soc.,2019

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