Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Rino, Bandiera"'
Autor:
Claudia, Mignone, Maura, Sandri, Rino, Bandiera, Bogliolo, Alessandro, Silvia, Casu, Maria Teresa Fulco, Giuliana, Giobbi, Klopfenstein, CUNO LORENZ, Leonardi, Laura, Marco, Malaspina, Rachele, Toniolo, Ginevra, Trinchieri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3656::4e61b84c992ea0b6ae372a08982a71a4
https://hdl.handle.net/11576/2707470
https://hdl.handle.net/11576/2707470
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Understanding the evolution of a supernova remnant shell in time is fundamental. Such understanding is critical to build reliable models of the dynamics of the supernova remnant shell interaction with any pulsar wind nebula it might contain. Here, we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0b230255c231fc2ce3c2bb8d43026e21
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The standard approach to the long-term evolution of pulsar wind nebulae (PWNe) is based on one-zone models treating the nebula as a uniform system. In particular for the late phase of evolved systems, many of the generally used prescriptions are base
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7132d20fa6bca537f03afd716b4b02a1
http://arxiv.org/abs/2009.10992
http://arxiv.org/abs/2009.10992
The analysis of Balmer-dominated emission in supernova remnants is potentially a very powerful way to derive information on the shock structure, on the physical conditions of the ambient medium and on the cosmic-ray acceleration efficiency. However,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f630cd284bd8c49e43d0e313ff73bad
http://hdl.handle.net/20.500.12386/29500
http://hdl.handle.net/20.500.12386/29500
Autor:
I. De Looze, F. D. Priestley, A. Bevan, M. J. Barlow, Mikako Matsuura, Haley Louise Gomez, Michael Bietenholz, Rino Bandiera, H. Chawner, Roger Wesson
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We have modelled the near-infrared to radio images of the Crab Nebula with a Bayesian SED model to simultaneously fit its synchrotron, interstellar and supernova dust emission. We infer an interstellar dust extinction map with an average $A_{\text{V}
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13cadf65de13b661289f95c706dac7e8
https://biblio.ugent.be/publication/8694949/file/8713589
https://biblio.ugent.be/publication/8694949/file/8713589
Polarized radio emission has been mapped with great detail in several Galactic supernova remnants (SNRs), but has not yet been exploited to the extent it deserves. We have developed a method to model maps of the Stokes parameters for shell-like SNRs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::007e8e7203c8fc54f553e60c0c52f5fb
http://arxiv.org/abs/1705.05803
http://arxiv.org/abs/1705.05803
Publikováno v:
IAU Symposium 331 : SN 1987A, 30 Years Later
IAU Symposium 331 : SN 1987A, 30 Years Later, Feb 2017, Saint-Gilles-les-Bains, La Réunion, France. pp.63-68, ⟨10.1017/S1743921317004756⟩
IAU Symposium 331 : SN 1987A, 30 Years Later, Feb 2017, Saint-Gilles-les-Bains, La Réunion, France. pp.63-68, ⟨10.1017/S1743921317004756⟩
A large fraction of core-collapse supernovae are thought to result in the birth of a rotation-powered pulsar, which is later observable as a radio pulsar up to great ages. The birth properties of these pulsars, and in particular the distribution of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2df85486b4357fd06dd2ec13cbe6da4
https://hal.archives-ouvertes.fr/hal-02136846
https://hal.archives-ouvertes.fr/hal-02136846
Autor:
Rino Bandiera, Oleh Petruk
The maps of intensity and polarization of the radio synchrotron emission from shell-type supernova remnants (SNRs) contain a considerable amount of information, although of not easy interpretation. With the aim of deriving constraints on the 3-D spat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8cf1e079aea27c2ca3ae2276ff2b26d
http://hdl.handle.net/20.500.12386/29514
http://hdl.handle.net/20.500.12386/29514
Publikováno v:
Advances in Space Research. 41:407-410
The investigation of the general properties of non-thermal (NT) X-ray shell supernova remnants (SNRs), of which SN 1006 is the prototype, is important to understand how electrons are accelerated in SNR shocks and what is the origin of cosmic rays. Us
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c022c98f731a15f143beaca60ef243bf
https://doi.org/10.1016/j.asr.2007.06.036
https://doi.org/10.1016/j.asr.2007.06.036
Pulsar wind nebulae are among the most powerful particle accelerators in the Galaxy with acceleration efficiencies that reach up to 30% and maximum particle energies in the PeV range. In recent years relativistic axisymmetric MHD models have proven t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef96dccc482e3abcc7896768d63234f1
http://hdl.handle.net/20.500.12386/23641
http://hdl.handle.net/20.500.12386/23641