Zobrazeno 1 - 4
of 4
pro vyhledávání: '"individual: Crab Nebula [supernovae]"'
Autor:
Dmitry Khangulyan, Diego F. Torres, E. de Oña Wilhelmi, Enrique Mestre, Fabio Acero, Roberta Zanin
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501 (1), pp.337-346. ⟨10.1093/mnras/staa3599⟩
Monthly notices of the Royal Astronomical Society 509(1), 337-346 (2020). doi:10.1093/mnras/staa3599
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 2021, 501 (1), pp.337-346. ⟨10.1093/mnras/staa3599⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501 (1), pp.337-346. ⟨10.1093/mnras/staa3599⟩
Monthly notices of the Royal Astronomical Society 509(1), 337-346 (2020). doi:10.1093/mnras/staa3599
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 2021, 501 (1), pp.337-346. ⟨10.1093/mnras/staa3599⟩
Monthly notices of the Royal Astronomical Society 509(1), 337 - 346 (2020). doi:10.1093/mnras/staa3599
Since 2009, several rapid and bright flares have been observed at high energies (>100 MeV) from the direction of the Crab Nebula. Several hypo
Since 2009, several rapid and bright flares have been observed at high energies (>100 MeV) from the direction of the Crab Nebula. Several hypo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f50b44cc3d65148c8c2187acedbb08eb
https://hal.archives-ouvertes.fr/hal-03070605
https://hal.archives-ouvertes.fr/hal-03070605
Autor:
S. Lombardi, O. Catalano, S. Scuderi, L. A. Antonelli, G. Pareschi, E. Antolini, L. Arrabito, G. Bellassai, K. Bernlöhr, C. Bigongiari, B. Biondo, G. Bonanno, G. Bonnoli, G. M. Böttcher, J. Bregeon, P. Bruno, R. Canestrari, M. Capalbi, P. Caraveo, P. Conconi, V. Conforti, G. Contino, G. Cusumano, E. M. de Gouveia Dal Pino, A. Distefano, G. Farisato, C. Fermino, M. Fiorini, A. Frigo, S. Gallozzi, C. Gargano, S. Garozzo, F. Gianotti, S. Giarrusso, R. Gimenes, E. Giro, A. Grillo, D. Impiombato, S. Incorvaia, N. La Palombara, V. La Parola, G. La Rosa, G. Leto, F. Lucarelli, M. C. Maccarone, D. Marano, E. Martinetti, A. Miccichè, R. Millul, T. Mineo, G. Nicotra, G. Occhipinti, I. Pagano, M. Perri, G. Romeo, F. Russo, B. Sacco, P. Sangiorgi, F. G. Saturni, A. Segreto, G. Sironi, G. Sottile, A. Stamerra, L. Stringhetti, G. Tagliaferri, M. Tavani, V. Testa, M. C. Timpanaro, G. Toso, G. Tosti, M. Trifoglio, G. Umana, S. Vercellone, R. Zanmar Sanchez, C. Arcaro, A. Bulgarelli, M. Cardillo, E. Cascone, A. Costa, A. D’Aì, F. D’Ammando, M. Del Santo, V. Fioretti, A. Lamastra, S. Mereghetti, F. Pintore, G. Rodeghiero, P. Romano, J. Schwarz, E. Sciacca, F. R. Vitello, A. Wolter
Publikováno v:
Astron.Astrophys.
Astron.Astrophys., 2020, 634, pp.A22. ⟨10.1051/0004-6361/201936791⟩
Astron.Astrophys., 2020, 634, pp.A22. ⟨10.1051/0004-6361/201936791⟩
We report on the first detection of very high-energy (VHE) gamma-ray emission from the Crab Nebula by a Cherenkov telescope in dual-mirror Schwarzschild-Couder (SC) configuration. The result has been achieved by means of the 4 m size ASTRI-Horn teles
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea9e242032010fcaa8cdd7890289b7ab
https://hal.archives-ouvertes.fr/hal-02381999
https://hal.archives-ouvertes.fr/hal-02381999
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
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 492 (1), pp.708-718. ⟨10.1093/mnras/stz3421⟩
Monthly notices of the Royal Astronomical Society 492(1), 708-718 (2020). doi:10.1093/mnras/stz3421
instname
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 492 (1), pp.708-718. ⟨10.1093/mnras/stz3421⟩
Monthly notices of the Royal Astronomical Society 492(1), 708-718 (2020). doi:10.1093/mnras/stz3421
The Cherenkov Telescope Array (CTA) will be the next generation instrument for the very high energy gamma-ray astrophysics domain. With its enhanced sensitivity in comparison with the current facilities, CTA is expected to shed light on a varied popu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c5f2dedc548a28ed5b499f9ecd2485a
http://hdl.handle.net/10261/237197
http://hdl.handle.net/10261/237197