Zobrazeno 1 - 10
of 139
pro vyhledávání: '"Piovan L"'
Autor:
Pasetto, S., Grebel, E. K., Chiosi, C., Crnojevic, D., Zeidler, P., Busso, G., Cassara, L. P., Piovan, L., Tantalo, R., Brogliato, C.
We present a new Galaxy population synthesis Model (GalMod). GalMod is a star-count model featuring an asymmetric bar/bulge as well as spiral arms and related extinction. The model, initially introduced in Pasetto et al. (2016b), has been here comple
Externí odkaz:
http://arxiv.org/abs/1805.00486
In this paper we explore the possibility that isolated CO-WDs with mass smaller than the Chandrasekhar limit may undergo nuclear runaway and SNa explosion, triggered by the energy produced by under-barrier pycno-nuclear reactions between carbon and l
Externí odkaz:
http://arxiv.org/abs/1409.1104
We investigate the influence of Asymptotic Giant Branch stars on integrated colours of star clusters of ages between ~100 Myr and a few gigayears, and composition typical for the Magellanic Clouds. We use state-of-the-art stellar evolution models tha
Externí odkaz:
http://arxiv.org/abs/1403.2505
We have employed state-of-the-art evolutionary models of low and intermediate-mass AGB stars, and included the effect of circumstellar dust shells on the spectral energy distribution (SED) of AGB stars, to revise the Padua library of isochrones (Bert
Externí odkaz:
http://arxiv.org/abs/1309.5938
Models of chemical evolution of galaxies including the dust are nowadays required to decipher the high-z universe. In a series of three papers we have tackled the problem and set a modern chemical evolution model. In the first paper (Piovan et al., 2
Externí odkaz:
http://arxiv.org/abs/1107.4567
Over the past decade a new generation of chemical models have included the dust in the treatment of the ISM. This major accomplishment has been spurred by the growing amounts of data on the highly obscured high-z Universe and the intriguing local pro
Externí odkaz:
http://arxiv.org/abs/1107.4561
The growing interest in the high-z universe, where strongly obscured objects are present, has determined an effort to improve the simulations of dust formation and evolution in galaxies. Three main basic ingredients enter the problem influencing the
Externí odkaz:
http://arxiv.org/abs/1107.4541
Modelling the complex physics of the Interstellar Medium (ISM) in the context of large-scale numerical simulations is a challenging task. A number of methods have been proposed to embed a description of the ISM into different codes. We propose a new
Externí odkaz:
http://arxiv.org/abs/1103.0509
We present ROBO, a model and its companion code for the study of the interstellar medium (ISM). The aim is to provide an accurate description of the physical evolution of the ISM and to set the ground for an ancillary tool to be inserted in NBody-Tre
Externí odkaz:
http://arxiv.org/abs/1012.1142
Autor:
Marino, A., Iodice, E., Tantalo, R., Piovan, L., Bettoni, D., Buson, L. M., Chiosi, C., Galletta, G., Rampazzo, R., Rich, R. M.
Systems of shells and polar rings in early-type galaxies are considered "bona fide" tracers of mass accretion and/or mergers. Their high frequency in low density environments suggests that such episodes could drive the evolution of at least a fractio
Externí odkaz:
http://arxiv.org/abs/0909.4020