Zobrazeno 1 - 10
of 77
pro vyhledávání: '"S. Loru"'
Autor:
A. Y. Ibrahim, A. Borghese, N. Rea, F. Coti Zelati, E. Parent, T. D. Russell, S. Ascenzi, R. Sathyaprakash, D. Götz, S. Mereghetti, M. Topinka, M. Rigoselli, V. Savchenko, S. Campana, G. L. Israel, A. Tiengo, R. Perna, R. Turolla, S. Zane, P. Esposito, G. A. Rodríguez Castillo, V. Graber, A. Possenti, C. Dehman, M. Ronchi, S. Loru
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 1, p 20 (2023)
Swift J1818.0−1607 is a radio-loud magnetar with a spin period of 1.36 s and a dipolar magnetic field strength of B ∼ 3 × 10 ^14 G, which is very young compared to the Galactic pulsar population. We report here on the long-term X-ray monitoring
Externí odkaz:
https://doaj.org/article/a93adba7d7d34265a25f844cd5655eb5
Autor:
O Petruk, V Beshley, S Orlando, F Bocchino, M Miceli, S Nagataki, M Ono, S Loru, A Pellizzoni, E Egron
The detected polarized radio emission from remnant of SN1987A opens the possibility to unveil the structure of the pre-supernova magnetic field in the circumstellar medium. Properties derived from direct measurements would be of importance for unders
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ded1c34964c449e9655c527d52f270e
https://hdl.handle.net/10447/588814
https://hdl.handle.net/10447/588814
Akademický článek
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Akademický článek
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Autor:
A. Y. Ibrahim, A. Borghese, N. Rea, F. Coti Zelati, E. Parent, T. D. Russell, S. Ascenzi, R. Sathyaprakash, D. Götz, S. Mereghetti, M. Topinka, M. Rigoselli, V. Savchenko, S. Campana, G. L. Israel, A. Tiengo, R. Perna, R. Turolla, S. Zane, P. Esposito, G. A. Rodríguez Castillo, V. Graber, A. Possenti, C. Dehman, M. Ronchi, S. Loru
Publikováno v:
Astrophys.J.
Astrophys.J., 2023, 943 (1), pp.20. ⟨10.3847/1538-4357/aca528⟩
Astrophys.J., 2023, 943 (1), pp.20. ⟨10.3847/1538-4357/aca528⟩
Swift J1818.0-1607 is a radio-loud magnetar with a spin period of 1.36 s and a dipolar magnetic field strength of B~3E14 G, which is very young compared to the Galactic pulsar population. We report here on the long-term X-ray monitoring campaign of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c4bd00869b230cc6da0733cd33dc999
http://arxiv.org/abs/2211.12391
http://arxiv.org/abs/2211.12391
Autor:
Paolo Leto, Neil M. Phillips, Filomena Bufano, C. Agliozzo, Jiří Krtička, F. Cavallaro, L. Cerrigone, Matt Shultz, Corrado Trigilio, Francesco Leone, G. Umana, M. Giarrusso, Luca Fossati, Carla Buemi, Ignazio Pillitteri, Jan Robrade, Richard Ignace, C. Bordiu, Helge Todt, A. Ingallinera, S. Loru, L. M. Oskinova, Simone Riggi
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:1979-1998
In this paper, we present the analysis of incoherent non-thermal radio emission from a sample of hot magnetic stars, ranging from early-B to early-A spectral type. Spanning a wide range of stellar parameters and wind properties, these stars display a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ece6100f28e3a96e07dbc7b003c40267
https://doi.org/10.1093/mnras/stab2168
https://doi.org/10.1093/mnras/stab2168
Autor:
P Leto, L M Oskinova, C S Buemi, M E Shultz, F Cavallaro, C Trigilio, G Umana, L Fossati, I Pillitteri, J Krtička, R Ignace, C Bordiu, F Bufano, G Catanzaro, L Cerrigone, M Giarrusso, A Ingallinera, S Loru, S P Owocki, K A Postnov, S Riggi, J Robrade, F Leone
KQVel is a binary system composed of a slowly rotating magnetic Ap star with a companion of unknown nature. In this paper, we report the detection of its radio emission. We conducted a multi-frequency radio campaign using the ATCA interferometer (ban
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::44c4f66d5532999e8df8e8acca3ed449
http://arxiv.org/abs/2207.14075
http://arxiv.org/abs/2207.14075
Akademický článek
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Autor:
A. Pellizzoni, S. Righini, M. N. Iacolina, M. Marongiu, S. Mulas, G. Murtas, G. Valente, E. Egron, M. Bachetti, F. Buffa, R. Concu, G. L. Deiana, S. L. Guglielmino, A. Ladu, S. Loru, A. Maccaferri, P. Marongiu, A. Melis, A. Navarrini, A. Orfei, P. Ortu, M. Pili, T. Pisanu, G. Pupillo, A. Saba, L. Schirru, G. Serra, C. Tiburzi, A. Zanichelli, P. Zucca, M. Messerotti
We present a new solar radio imaging system implemented through the upgrade of the large single-dish telescopes of the Italian National Institute for Astrophysics (INAF), not originally conceived for solar observations. During the development and ear
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2fcc87f12843f90891d9ff49c0ff1702
http://arxiv.org/abs/2205.00197
http://arxiv.org/abs/2205.00197
Autor:
A Ingallinera, F Cavallaro, S Loru, J Marvil, G Umana, C Trigilio, S Breen, C Bordiu, C S Buemi, F Bufano, J Collier, S Etoka, M D Filipović, S R Goldman, A M Hopkins, B S Koribalski, P Leto, R P Norris, S Riggi, F Schillirò, C Tremblay, J Th van Loon
Low- and intermediate-mass stars end their life dispersing their outer layers into the circumstellar medium, during the asymptotic and post-asymptotic giant branch phases. OH masers at 18 cm offer an effective way to probe their circumstellar environ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cceb56b717c7f91a34d2b2a12e580cfc
http://hdl.handle.net/20.500.12386/32886
http://hdl.handle.net/20.500.12386/32886