Zobrazeno 1 - 10
of 143
pro vyhledávání: '"Amedeo Tornambe"'
We investigate the evolutionary properties of AM~CVn stars with massive white dwarf donors and accretors. As a representative of them we consider a binary initially composed by a 0.30 M$_\odot$, He WD and a 1.02 M$_\odot$, CO WD. We evaluate the time
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b9f9aca8c839a7d1c50aecf8bb7e1ed9
http://hdl.handle.net/20.500.12386/28671
http://hdl.handle.net/20.500.12386/28671
We determine the expected signal in various observational bands of Supernovae Ia progenitors just before the explosion by assuming the rotating Double Degenerate scenario. Our results are valid also for all the evolutionary scenarios invoking rotatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::574dd117ff759ffe547b2cd62aa34739
http://hdl.handle.net/20.500.12386/28665
http://hdl.handle.net/20.500.12386/28665
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 452:2897-2910
We study the physical and evolutionary properties of the "WD family" of AM CVn stars by computing realistic models of IDD systems. We evaluate self-consistently both the mass transfer rate from the donor, as determined by GW emission and interaction
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7679d3d26c41f608e05e94c6876c6ca
https://doi.org/10.1093/mnras/stv1452
https://doi.org/10.1093/mnras/stv1452
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 445:3239-3262
The behaviour of carbon-oxygen white dwarfs (WDs) subject to direct helium accretion is extensively studied. We aim to analyze the thermal response of the accreting WD to mass deposition at different time scales. The analysis has been performed for i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1d640b06b0304e3cf0d90b92b5877dbd
https://doi.org/10.1093/mnras/stu1885
https://doi.org/10.1093/mnras/stu1885
Autor:
Amedeo Tornambe, Roberto Maiolino, Rosa Valiante, Francesca D'Antona, Simona Gallerani, Paolo Ventura, M. Di Criscienzo, R. Carini, Raffaella Schneider
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 424:2345-2357
We calculate the dust formed around AGB and SAGB stars of metallicity Z=0.008 by following the evolution of models with masses in the range 1M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b733d220e0e9d5e688ca45a2b5652323
https://doi.org/10.1111/j.1365-2966.2012.21403.x
https://doi.org/10.1111/j.1365-2966.2012.21403.x
Autor:
Rosa Valiante, R. Carini, Amedeo Tornambe, Paolo Ventura, Raffaella Schneider, Simona Gallerani, M. Di Criscienzo, Roberto Maiolino, F. D'Antona
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 420:1442-1456
We compute the mass and composition of dust produced by stars with masses in the range and with a metallicity of Z= 0.001 during their asymptotic giant branch (AGB) and super-AGB phases. Stellar evolution is followed from the pre-main-sequence phase
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7fb34b2952103b2a703eedf01ab72a3f
https://doi.org/10.1111/j.1365-2966.2011.20129.x
https://doi.org/10.1111/j.1365-2966.2011.20129.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 353:243-248
This paper addresses the problem of pseudo-evolutionary zero-age horizontal branch (ZAHB) models, as produced in the current literature, starting from suitable assumptions about the post-He flash structures. To test the accuracy of this procedure, we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4cce865553bed1fdbd2a3397a273c200
https://doi.org/10.1111/j.1365-2966.2004.08064.x
https://doi.org/10.1111/j.1365-2966.2004.08064.x
Autor:
Itziar Aretxaga, Gaetano Valentini, A. Caratti, I. J. Danziger, Enrico Cappellaro, A. Pastorello, Mauro Dolci, Valeri M. Larionov, Amedeo Tornambe, Yu. N. Gnedin, Massimo Turatto, G. Li Causi, Olga Vega, Roberto Speziali, Francesco D'Alessio, Fernando Pedichini, S. Benetti, E. Di Carlo, A. A. Arkharov, A. Di Paola, Enzo Brocato, D. Guidubaldi, F. Massi, V. H. Chavushyan
Publikováno v:
The Astrophysical Journal. 573:144-156
Optical and near-infrared light curves of the Type IIn supernova 1999el in NGC 6951 are presented. A period of 220 days (416 days in the near-infrared) is covered from the first observation obtained a few days before maximum light. Spectroscopic obse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::080ab404b16b088ce644dcee2641715f
https://doi.org/10.1086/340496
https://doi.org/10.1086/340496
Autor:
Amedeo Tornambe, Luciano Piersanti, Gabriel Martínez-Pinedo, Oscar Straniero, Inmaculada Domínguez, Sergio Cristallo, Eduardo Bravo
Publikováno v:
Recercat. Dipósit de la Recerca de Catalunya
instname
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
instname
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
The ultimate understanding of SNe Ia diversity is one of the most urgent issues to exploit thermonuclear explosions of accreted White Dwarfs (WDs) as cosmological yardsticks. In particular, we investigate the impact of the progenitor system metallici
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79018ff2ad6a29b8e6bac0ac5ba3ceb2
https://doi.org/10.3847/2041-8213/aa5c7e
https://doi.org/10.3847/2041-8213/aa5c7e
Autor:
Pierluigi Monaco, Fabio Fontanot, Barbara Lo Faro, Gabriella De Lucia, Eros Vanzella, Rachel Somerville, Stefano Cristiani, Laura Silva, Paola Santini, Giuliana Giobbi, Amedeo Tornambe, Gabriella Raimondo, Marco Limongi, L. A. Antonelli, Nicola Menci, Enzo Brocato
By comparing galaxy formation models within the ΛCDM cosmology with available data on high redshift galaxies, we show that small galaxies , with stellar masses
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::60cf95afac32b5fd1debe14d6fa5a6f5
https://hdl.handle.net/11368/2633323
https://hdl.handle.net/11368/2633323