Zobrazeno 1 - 10
of 11 736
pro vyhledávání: '"Bocchino A"'
Autor:
Chiara Abiuso
Publikováno v:
Estudios de Teoría Literaria, Vol 10, Iss 23, Pp 232-235 (2021)
Bibliogrphic review of Adriana A. Bocchino y Esteban Prado (coords.) Nuevos objetos/Nuevas teorías. Teorías críticas sobre el presente. Mar del Plata, Eudem, 2020, 307 pp.
Externí odkaz:
https://doaj.org/article/e60db1c096bd449f8bba5b8c6f822492
Autor:
Orlando, S., Greco, E., Hirai, R., Matsuoka, T., Miceli, M., Nagataki, S., Ono, M., Chen, K. -J., Milisavljevic, D., Patnaude, D., Bocchino, F., Elias-Rosa, N.
We investigate SN 2014C using three-dimensional hydrodynamic modeling, focusing on its early interaction with dense circumstellar medium (CSM). Our objective is to uncover the pre-supernova (SN) CSM structure and constrain the progenitor star's mass-
Externí odkaz:
http://arxiv.org/abs/2410.17699
Autor:
Orlando, S., Miceli, M., Patnaude, D. J., Plucinsky, P. P., Lee, S. -H., Badenes, C., Janka, H. -T., Wongwathanarat, A., Raymond, J., Sasaki, M., Churazov, E., Khabibullin, I., Bocchino, F., Castro, D., Millard, M.
(Abridged) Core-collapse supernova remnants (SNRs) display complex morphologies and asymmetries, reflecting anisotropies from the explosion and early interactions with the circumstellar medium (CSM). Spectral analysis of these remnants can provide cr
Externí odkaz:
http://arxiv.org/abs/2408.12462
Autor:
Sapienza, Vincenzo, Miceli, Marco, Petruk, Oleh, Bamba, Aya, Katsuda, Satoru, Orlando, Salvatore, Bocchino, Fabrizio, DeLaney, Tracey
The maximum energy of electrons in supernova remnant (SNR) shocks is typically limited by radiative losses, where the synchrotron cooling time equals the acceleration time. The low speed of shocks in a dense medium increases the acceleration time, le
Externí odkaz:
http://arxiv.org/abs/2407.18980
Autor:
Petruk, Oleh, Kuzyo, Taras, Patrii, Mariana, Chomiuk, Laura, Arias, Maria, Miceli, Marco, Orlando, Salvatore, Bocchino, Fabrizio
By using surface brightness maps of Tycho's supernova remnant (SNR) in radio and X-rays, along with the properties of thermal and synchrotron emission, we have derived the post-shock density and magnetic field strength distributions over the projecti
Externí odkaz:
http://arxiv.org/abs/2407.10929
Publikováno v:
Il Foro Italiano, 2014 Sep 01. 137(9), 2541/2542-2553/2554.
Externí odkaz:
https://www.jstor.org/stable/44879320
Autor:
Palmieri, A.
Publikováno v:
Il Foro Italiano, 2013 Jul 01. 136(7/8), 2171/2172-2175/2176.
Externí odkaz:
https://www.jstor.org/stable/23730180
Autor:
Bark, Jamil Mamedio, 1964
Publikováno v:
Repositório Institucional da UnicampUniversidade Estadual de CampinasUNICAMP.
Orientador: Mauricy Matos Martin
Dissertação (mestrado) - Universidade Estadual de Campinas, Instituto de Artes
Made available in DSpace on 2018-08-27T04:27:50Z (GMT). No. of bitstreams: 1 Bark_JamilMamedio_M.pdf: 18908239 bytes, checksum
Dissertação (mestrado) - Universidade Estadual de Campinas, Instituto de Artes
Made available in DSpace on 2018-08-27T04:27:50Z (GMT). No. of bitstreams: 1 Bark_JamilMamedio_M.pdf: 18908239 bytes, checksum
Externí odkaz:
http://repositorio.unicamp.br/jspui/handle/REPOSIP/284985
Autor:
Sapienza, Vincenzo, Miceli, Marco, Bamba, Aya, Orlando, Salvatore, Lee, Shiu-Hang, Nagataki, Shigehiro, Ono, Masaomi, Katsuda, Satoru, Mori, Koji, Sawada, Makoto, Terada, Yukikatsu, Giuffrida, Roberta, Bocchino, Fabrizio
Supernova (SN) 1987A is widely regarded as an excellent candidate for leveraging the capabilities of the freshly launched XRISM satellite. Recent researches indicate that the X-ray emission from SN 1987A will increasingly originate from its ejecta in
Externí odkaz:
http://arxiv.org/abs/2406.00090
Publikováno v:
Il Foro Italiano, 2012 Jun 01. 135(6), 1759/1760-1765/1766.
Externí odkaz:
https://www.jstor.org/stable/26638831