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pro vyhledávání: '"Yasuda, Haruo"'
Autor:
Yasuda, Haruo
甲第23706号
理博第4796号
新制||理||1686(附属図書館)
(主査)講師 LEE Shiu Hang, 教授 嶺重 慎, 准教授 前田 啓一
学位規則第4条第1項該当
Doctor of Science
Kyoto University
DFAM
理博第4796号
新制||理||1686(附属図書館)
(主査)講師 LEE Shiu Hang, 教授 嶺重 慎, 准教授 前田 啓一
学位規則第4条第1項該当
Doctor of Science
Kyoto University
DFAM
Externí odkaz:
http://hdl.handle.net/2433/275028
The contribution of galactic supernova remnants (SNRs) to the origin of cosmic rays (CRs) is an important open question in modern astrophysics. Broadband non-thermal emission is a useful proxy for probing the energy budget and production history of C
Externí odkaz:
http://arxiv.org/abs/2207.06203
Supernova remnants (SNRs) are important objects in investigating the links among supernova (SN) explosion mechanism(s), progenitor stars, and cosmic-ray acceleration. Non-thermal emission from SNRs is an effective and promising tool for probing their
Externí odkaz:
http://arxiv.org/abs/2111.09534
Supernova remnants (SNRs) are important objects in terms of their connections with supernova (SN) explosion mechanism(s), progenitor stars, and cosmic-ray acceleration. Non-thermal emission from SNRs is an effective probe of the structure of their su
Externí odkaz:
http://arxiv.org/abs/2109.04032
Recent high-cadence transient surveys and rapid follow-up observations indicate that some massive stars may dynamically lose their own mass within decades before supernovae (SNe). Such a mass-loss forms `confined' circumstellar medium (CSM); a high d
Externí odkaz:
http://arxiv.org/abs/1909.05874
Autor:
Yasuda, Haruo, Lee, Shiu-Hang
Supernova remnants (SNRs) are thought to be one of the major acceleration sites of galactic cosmic rays (CRs) and an important class of objects for high-energy astrophysics. SNRs produce multi-wavelength, non-thermal emission via accelerated particle
Externí odkaz:
http://arxiv.org/abs/1903.10226
Akademický článek
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Publikováno v:
Astrophysical Journal; 9/1/2022, Vol. 936 Issue 1, p1-20, 20p
Publikováno v:
Astrophysical Journal. 876
Supernova remnants (SNRs) are thought to be one of the major acceleration sites of galactic cosmic rays and an important class of objects for high-energy astrophysics. SNRs produce multiwavelength, nonthermal emission via accelerated particles at col
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::9cfc7a71100023e4013135bb9aff1c6c
http://hdl.handle.net/2433/243154
http://hdl.handle.net/2433/243154