Výsledky vyhledávání - "G. B. Pisani"

The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs

Autor: L. Becerra, Christian Cherubini, Grant J. Mathews, Y. Aimuratov, Narek Sahakyan, Rahim Moradi, Jorge A. Rueda, G. B. Pisani, R. Ruffini, Marco Muccino, S. S. Xue, Carlo Luciano Bianco, Y. Wang, L. Li, M. Karlica, Simonetta Filippi, Y. C. Chen

Publikováno v: Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, ⟨10.1093/mnras/stab724⟩

We recall evidence that long gamma-ray bursts (GRBs) have binary progenitors and give new examples. Binary-driven hypernovae (BdHNe) consist of a carbon-oxygen core (CO$_{\rm core}$) and a neutron star (NS) companion. For binary periods $\sim 5$ min,

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a740b298d8a829264d6ff113c4f0b72
https://hal.archives-ouvertes.fr/hal-03186184

Zobrazit plný text záznamu

The binary progenitors of short and long GRBs and their gravitational-wave emission

Autor: Marco Muccino, U. Barres de Almeida, Christian Cherubini, Jorge A. Rueda, Rahim Moradi, Carlo Luciano Bianco, Remo Ruffini, Milos Kovacevic, J. F. Rodriguez, L. Becerra, Y. Aimuratov, G. B. Pisani, Y. Wang, Simonetta Filippi

Publikováno v: EPJ Web Conf.
13th International Conference on Gravitation, Astrophysics and Cosmology and 15th Italian-Korean Symposium on Relativistic Astrophysics
13th International Conference on Gravitation, Astrophysics and Cosmology and 15th Italian-Korean Symposium on Relativistic Astrophysics, Jul 2017, Seoul, South Korea. pp.01006, ⟨10.1051/epjconf/201816801006⟩
EPJ Web of Conferences, Vol 168, p 01006 (2018)

International audience; We have sub-classified short and long-duration gamma-ray bursts (GRBs) into seven families according to the binary nature of their progenitors. Short GRBs are produced in mergers of neutron-star binaries (NS-NS) or neutron sta

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc602e447591b2f912d99101a10f8649
https://hal.archives-ouvertes.fr/hal-01757957

Zobrazit plný text záznamu

Evolution of an electron-positron plasma produced by induced gravitational collapse in binary-driven hypernovae

Autor: J. D. Melon Fuksman, Milos Kovacevic, M. Karlica, Marco Muccino, G. B. Pisani, Rahim Moradi, Remo Ruffini, Carlo Luciano Bianco, Jorge A. Rueda, D. Primorac, Y. Wang, L. Becerra, Gregory Vereshchagin

Publikováno v: EPJ Web Conf.
13th International Conference on Gravitation, Astrophysics and Cosmology and 15th Italian-Korean Symposium on Relativistic Astrophysics
13th International Conference on Gravitation, Astrophysics and Cosmology and 15th Italian-Korean Symposium on Relativistic Astrophysics, Jul 2017, Seoul, South Korea. pp.04009, ⟨10.1051/epjconf/201816804009⟩
EPJ Web of Conferences, Vol 168, p 04009 (2018)

The binary-driven hypernova (BdHN) model has been introduced in the past years, to explain a subfamily of gamma-ray bursts (GRBs) with energies Eiso ≥ 1052 erg associated with type Ic supernovae. Such BdHNe have as progenitor a tight binary system

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a2da9ac04632414e7d3dfaff46e4c2c
https://hal.archives-ouvertes.fr/hal-01757956

Zobrazit plný text záznamu

Vyhledávací nástroje:

Upřesnit hledání