Search Results - "Marassi, S"

Where does galactic dust come from? by Ginolfi, M., Graziani, L., Schneider, R., Marassi, S., Valiante, R., Dell'Agli, F., Ventura, P., Hunt, L. K.

“…AbstractHere we investigate the origin of the dust mass (Mdust ) observed in the Milky Way (MW) and of dust scaling relations found in a sample of local…”
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Cosmic archaeology with massive stellar black hole binaries by Graziani, L, Schneider, R, Marassi, S, Del Pozzo, W, Mapelli, M, Giacobbo, N

“…ABSTRACT The existence of massive stellar black hole binaries (MBHBs), with primary black hole masses $\ge 31 \, \mathrm{ M}_\odot$, was proven by the…”
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Evolution of dwarf galaxies hosting GW150914-like events by Marassi, S, Graziani, L, Ginolfi, M, Schneider, R, Mapelli, M, Spera, M, Alparone, M

“…ABSTRACT Here we present a detailed analysis of the properties and evolution of different dwarf galaxies, candidates to host the coalescence of black hole…”
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THE ORIGIN OF THE MOST IRON-POOR STAR by Marassi, S, Chiaki, G, Schneider, R, Limongi, M, OMUKAI, K, Nozawa, T, Chieffi, A, TOSHIBA, N

“…We investigate the origin of carbon-enhanced metal-poor (CEMP) stars starting from the recently discovered [Fe/H] < -7.1 star SMSS J031300. We show that the…”
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Supernova dust yields: the role of metallicity, rotation, and fallback by Marassi, S, Schneider, R, Limongi, M, Chieffi, A, Graziani, L, Bianchi, S

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Deployment of in-body wearable devices in healthcare and at work: closing the EU regulatory gap by Marassi, S, Foldes, M E

“…Abstract Background In-body wearable devices can protect workers’ health and safety. Moreover, they might provide data that could be capitalized on in the…”
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Imprint of the merger and ring-down on the gravitational wave background from black hole binaries coalescence by Marassi, S., Schneider, R., Corvino, G., Ferrari, V., Zwart, S. Portegies

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Cosmic archaeology with massive stellar black hole binaries by Graziani, L, Schneider, R, Marassi, S, Del Pozzo, W, Mapelli, M, Giacobbo, N

“…The existence of massive stellar black hole binaries (MBHBs), with primary black hole (BH) masses $\ge 31 \, M_\odot$, was proven by the detection of the…”
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Evolution of dwarf galaxies hosting GW150914-like events by Marassi, S, Graziani, L, Ginolfi, M, Schneider, R, Mapelli, M, Spera, M, Alparone, M

“…Here we present a detailed analysis of the properties and evolution of different dwarf galaxies, candidate to host the coalescence of black hole binary systems…”
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Supernova dust yields: the role of metallicity, rotation, and fallback by Marassi, S, Schneider, R, Limongi, M, Chieffi, A, Graziani, L, Bianchi, S

“…Supernovae (SNe) are considered to have a major role in dust enrichment of high redshift galaxies and, due to the short lifetimes of interstellar grains, in…”
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Dust grains from the heart of supernovae by Bocchio, M, Marassi, S, Schneider, R, Bianchi, S, Limongi, M, Chieffi, A

“…Dust grains are classically thought to form in the winds of asymptotic giant branch (AGB) stars. However, there is increasing evidence today for dust formation…”
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Dust grains from the heart of supernovae by Bocchio, M, Marassi, S, Schneider, R, Bianchi, S, Limongi, M, Chieffi, A

“…Dust grains are classically thought to form in the winds of AGB stars. However, nowadays there is increasing evidence for dust formation in SNe. In order to…”
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The metal and dust yields of the first massive stars by Marassi, S, Schneider, R, Limongi, M, Chieffi, A, Bocchio, M, Bianchi, S

“…We quantify the role of Population (Pop) III core-collapse supernovae (SNe) as the first cosmic dust polluters. Starting from a homogeneous set of stellar…”
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Compact binaries detection rates from gravitational wave interferometers: comparison of different procedures by Corvino, G, Ferrari, V, Marassi, S, Schneider, R

“…In this paper we perform a detailed analysis of the effect of various approximations which have been used in the literature to compute the detection rates of…”
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Probing the High-Redshift Universe with SPICA: Toward the Epoch of Reionization and Beyond by Egami, E, Gallerani, S, Schneider, R, Pallottini, A, Vallini, L, Sobacchi, E, Ferrara, A, Bianchi, S, Bocchio, M, Marassi, S, Armus, L, Spinoglio, L, Blain, A. W, Bradford, M, Clements, D. L, Dannerbauer, H, Fernández-Ontiveros, J. A, González-Alfonso, E, Griffin, M. J, Gruppioni, C, Kaneda, H, Kohno, K, Madden, S. C, Matsuhara, H, Najarro, P, Nakagawa, T, Oliver, S, Omukai, K, Onaka, T, Pearson, C, Perez-Fournon, I, Pérez-González, P. G, Schaerer, D, Scott, D, Serjeant, S, Smith, J. D, van der Tak, F. F. S, Wada, T, Yajima, H

“…With the recent discovery of a dozen dusty star-forming galaxies and around 30 quasars at z>5 that are hyper-luminous in the infrared ($\mu$$L_{\rm…”
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A new approach to the study of quasi-normal modes of rotating stars by Ferrari, V, Gualtieri, L, Marassi, S

“…Phys.Rev.D76:104033,2007 We propose a new method to study the quasi-normal modes of rotating relativistic stars. Oscillations are treated as perturbations in…”
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Imprint of the merger and ring-down on the gravitational wave background from black hole binaries coalescence by Marassi, S, Schneider, R, Corvino, G, Ferrari, V, Zwart, S. Portegies

“…We compute the gravitational wave background (GWB) generated by a cosmological population of (BH-BH) binaries using hybrid waveforms recently produced by…”
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Galaxy evolution studies with the SPace IR telescope for Cosmology and Astrophysics (SPICA): the power of IR spectroscopy by Spinoglio, L, Alonso-Herrero, A, Armus, L, Baes, M, Bernard-Salas, J, Bianchi, S, Bocchio, M, Bolatto, A, Bradford, C. M, Braine, J, Carrera, F. J, Ciesla, L, Clements, D. L, Dannerbauer, H, Doi, Y, Efstathiou, A, Egami, E, Fernandez-Ontiveros, J. A, Ferrara, A, Fischer, J, Franceschini, A, Gallerani, S, Giard, M, Gonzalez-Alfonso, E, Gruppioni, C, Guillard, P, Hatziminaoglou, E, Imanishi, M, Ishihara, D, Isobe, N, Kaneda, H, Kawada, M, Kohno, K, Kwon, J, Madden, S, Malkan, M. A, Marassi, S, Matsuhara, H, Matsuura, M, Miniutti, G, Nagamine, K, Nagao, T, Najarro, F, Nakagawa, T, Onaka, T, Oyabu, S, Pallottini, A, Piro, L, Pozzi, F, Rodighiero, G, Roelfsema, P, Sakon, I, Santini, P, Schaerer, D, Schneider, R, Scott, D, Serjeant, S, Shibai, H, Smith, J. -D. T, Sobacchi, E, Sturm, E, Suzuki, T, Vallini, L, van der Tak, F, Vignali, C, Yamada, T, Wada, T, Wang, L

“…IR spectroscopy in the range 12-230 micron with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes that govern…”
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Perturbative approach to the structure of rapidly rotating neutron stars by Benhar, Omar, Ferrari, Valeria, Gualtieri, Leonardo, Marassi, Stefania

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