Zobrazeno 1 - 10
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pro vyhledávání: '"F., Pintore"'
Autor:
S., Scuderi, A., Giuliani, G., Pareschi, G., Tosti, O., Catalano, E., Amato, A., Antonelli L., J., Becerra Gonzáles, G., Bellassai, Bigongiari, B., Biondo, M., Böttcher, G., Bonanno, G., Bonnoli, P., Bruno, A., Bulgarelli, R., Canestrari, M., Capalbi, P., Caraveo, M., Cardillo, V., Conforti, G., Contino, M., Corpora, A., Costa, G., Cusumano, A., D'Aí, E., de Gouveia Dal Pino, R., Della Ceca, D., Escribano Rodriguez E. Falceta Gonçalves, C., Fermino, M., Fiori, V., Fioretti, M., Fiorini, S., Gallozzi, C., Gargano, S., Garozzo, S., Germani, A., Ghedina, F., Gianotti, S., Giarrusso, R., Gimenes, V., Giordano, A., Grillo, C., Grivel Gelly, D., Impiombato, F., Incardona, S., Incorvaia, S., Iovenitti, A., La Barbera, N., La Palombara, V., La Parola, A., Lamastra, L., Lessio, G., Leto, F., Lo Gerfo, M., Lodi, S., Lombardi, F., Longo, F., Lucarelli, C., Maccarone M., D., Marano, E., Martinetti, S., Mereghetti, A., Micciché, R., Millul, T., Mineo, D., Mollica, G., Morlino, A., Morselli, G., Naletto, G., Nicotra, A., Pagliaro, N., Parmiggiani, G., Piano, F., Pintore, E., Poretti, B., Olmi, G., Rodeghiero, G., Rodriguez Fernandez, P., Romano, G., Romeo, F., Russo, P., Sangiorgi, G., Saturni F., H., Schwarz J., Sciacca, G., Sironi, G., Sottile, A., Stamerra, G., Tagliaferri, V., Testa, G., Umana, M., Uslenghi, S., Vercellone, L., Zampieri, R, Zanmar Sanchez
Publikováno v:
Journal of High Energy Astrophysics, Volume 35, p. 52-68 (2022)
The ASTRI Mini-Array (MA) is an INAF project to build and operate a facility to study astronomical sources emitting at very high-energy in the TeV spectral band. The ASTRI MA consists of a group of nine innovative Imaging Atmospheric Cherenkov telesc
Externí odkaz:
http://arxiv.org/abs/2208.04571
Autor:
M Del Santo, C Pinto, A Marino, A D’Aì, P-O Petrucci, J Malzac, J Ferreira, F Pintore, S E Motta, T D Russell, A Segreto, A Sanna
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 523:L15-L20
The transient X-ray source MAXI J1810-222 was discovered in 2018 and has been active ever since. A long combined radio and X-ray monitoring campaign was performed with ATCA and Swift respectively. It has been proposed that MAXI J1810-222 is a relativ
Autor:
T D Russell, M Del Santo, A Marino, A Segreto, S E Motta, A Bahramian, S Corbel, A D’Aì, T Di Salvo, J C A Miller-Jones, C Pinto, F Pintore, A Tzioumis
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 513 (4), pp.6196-6209. ⟨10.1093/mnras/stac1332⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 2022, 513 (4), pp.6196-6209. ⟨10.1093/mnras/stac1332⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
We present results from radio and X-ray observations of the X-ray transient MAXI J1810-222. The nature of the accretor in this source has not been identified. In this paper, we show results from a quasi-simultaneous radio and X-ray monitoring campaig
Autor:
Chiara Salvaggio, A Wolter, F Pintore, C Pinto, E Ambrosi, G L Israel, A Marino, R Salvaterra, L Zampieri, A Belfiore
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:1814-1828
Variability is a powerful tool to investigate properties of X-ray binaries (XRB), in particular for Ultraluminous X-ray sources (ULXs) that are mainly detected in the X-ray band. For most ULXs the nature of the accretor is unknown, although a few ULX
Autor:
A Robba, C Pinto, F Pintore, G Rodriguez, E Ambrosi, F Barra, G Cusumano, A D’Aì, M Del Santo, P Kosec, A Marino, M Middleton, T Roberts, C Salvaggio, R Soria, A Wolter, D Walton
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2022, Vol.515(4), pp.4669-4674 [Peer Reviewed Journal]
Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10$^{39}$ erg s$^{-1}$. The average number of ULXs per galaxy is still not well constrained, especially given the uncertainty on the fraction of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::963c70cfd2e6882318bd70d00e74b242
http://arxiv.org/abs/2207.09447
http://arxiv.org/abs/2207.09447
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Autor:
S. Mereghetti, N. La Palombara, T. Kupfer, T. R. Marsh, C. M. Copperwheat, K. Deshmukh, P. Esposito, T. Maccarone, F. Pintore, M. Rigoselli, L. Rivera Sandoval, A. Tiengo
ZTF J213056.71+442046.5 is the prototype of a small class of recently discovered compact binaries composed of a white dwarf and a hot subdwarf that fills its Roche-lobe. Its orbital period of only 39 min is the shortest known for the objects in this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab75cfb22c05adb46a357c94468a0d86
http://wrap.warwick.ac.uk/167001/1/WRAP-X-ray-observation-of-the-Roche-lobe-filling-white-dwarf-plus-hot-subdwarf-system-ZTF-J213056.71-442046.5-Marsh-22.pdf
http://wrap.warwick.ac.uk/167001/1/WRAP-X-ray-observation-of-the-Roche-lobe-filling-white-dwarf-plus-hot-subdwarf-system-ZTF-J213056.71-442046.5-Marsh-22.pdf
Akademický článek
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