Zobrazeno 1 - 10
of 80
pro vyhledávání: '"Ignazio Pillitteri"'
Autor:
Nancy Remage Evans, H. Moritz Günther, Howard E. Bond, Gail H. Schaefer, Brian D. Mason, Margarita Karovska, Evan Tingle, Scott Wolk, Scott Engle, Edward Guinan, Ignazio Pillitteri, Charles Proffitt, Pierre Kervella, Alexandre Gallenne, Richard I. Anderson, Maxwell Moe
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 2, p 167 (2024)
Externí odkaz:
https://doaj.org/article/33e643295e5748ddbe7650e1a13c0af8
Autor:
Sabina Ustamujic, Salvatore Orlando, Laura Leonardi, Laura Daricello, Ignazio Pillitteri, Fabrizio Bocchino, Marco Miceli
Three-dimensional (3D) magnetohydrodynamic (MHD) simulations of astrophysical phenomena represent a challenge in standard data visualization for scientific purposes, for the amount of processed data and a wealth of scientific information they contain
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::08e093b57f94594c6487b7b0e51d6a0f
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:
Ignazio Pillitteri
Publikováno v:
Astronomische Nachrichten. 343
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fd8fc29ce76cdf97d57c0e12c5c75a3d
https://doi.org/10.1002/asna.20210099
https://doi.org/10.1002/asna.20210099
Hot Jupiters (HJs) are massive gaseous planets orbiting close to their host stars. Due to their physical characteristics and proximity to the central star, HJs are the natural laboratories to study the process of star-planet interaction (SPI). Phenom
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aade2307d6bb89c6b7a1a3185d3ab261
http://arxiv.org/abs/2111.11110
http://arxiv.org/abs/2111.11110
Publikováno v:
Astronomische Nachrichten. 340:334-339
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ec483ef2f89a9242ebcf9cc39c4b74d6
https://doi.org/10.1002/asna.201913620
https://doi.org/10.1002/asna.201913620
Autor:
Francesco Borsa, Silvano Desidera, Ignazio Pillitteri, Darius Modirrousta-Galian, Riccardo Claudi, Giuseppina Micela, S. Benatti, A. Maggio, D. Locci, L. Malavolta, Scott J. Wolk, Mario Damasso
We performed a radial velocity (RV) monitoring of the 40 Myr old star DS Tuc A with HARPS at the ESO-3.6m to determine the planetary mass of its 8.14-days planet, first revealed by TESS. We also observed two planetary transits with HARPS and ESPRESSO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e234a8191fc76b97a63e717f296e63e3
http://hdl.handle.net/11577/3415744
http://hdl.handle.net/11577/3415744
Autor:
Antonio Maggio, Laura Daricello, Laura Leonardi, Salvatore Orlando, Fabrizio Bocchino, Ignazio Pillitteri
Virtual reality (VR) devices allow the exploration of 3D data in a fully immersive fashion and make it possible to create a powerful engagement experience and a direct interaction with current scientific data to learn more about astronomy in Educatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cb618e133b598cf9ed148763143eab3c
https://doi.org/10.5194/epsc2020-1031
https://doi.org/10.5194/epsc2020-1031
Autor:
László Molnár, Edward F. Guinan, László Szabados, Róbert Szabó, Gilbert Burki, Vinay L. Kashyap, Hilding R. Neilson, Scott J. Wolk, H. Moritz Günther, Jeremy J. Drake, Nancy Remage Evans, Massimo Marengo, Peter Somogyi, Ignazio Pillitteri, Sofia P. Moschou, Lynn D. Matthews, Tamás Tordai, Pierre Kervella, Emese Plachy, Scott G. Engle
Publikováno v:
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2020, 159 (3), pp.121. ⟨10.3847/1538-3881/ab7121⟩
The Astronomical Journal, American Astronomical Society, 2020, 159 (3), pp.121. ⟨10.3847/1538-3881/ab7121⟩
V473 Lyr is a classical Cepheid which is unique in having substantial amplitude variations with a period of approximately 3.3 years, thought to be similar to the Blazhko variations in RR Lyrae stars. We obtained an {\it XMM-Newton} observation of thi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc0dcfc08660a1a3e13bd4aba9f3b337
https://hal.archives-ouvertes.fr/hal-03262839
https://hal.archives-ouvertes.fr/hal-03262839
Autor:
L. Cerrigone, Giovanni Catanzaro, Jan Robrade, S. Loru, C. Agliozzo, Filomena Bufano, Richard Ignace, A. Ingallinera, Neil M. Phillips, Corrado Trigilio, Francesco Leone, G. Umana, Ignazio Pillitteri, Paolo Leto, Luca Fossati, Francesco Schillirò, Simone Riggi, Jiri Krticka, L. M. Oskinova, F. Cavallaro, M. Giarrusso, Carla Buemi
The non-thermal radio emission of main-sequence early-type stars is a signature of stellar magnetism. We present multi-wavelength (1.6-16.7 GHz) ATCA measurements of the early-type magnetic star rho OphC, which is a flat-spectrum non-thermal radio so
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a00048dbb04eea4fc79c0ee7735c080a
http://hdl.handle.net/20.500.11769/487953
http://hdl.handle.net/20.500.11769/487953