Zobrazeno 1 - 10
of 332
pro vyhledávání: '"Rossi, Martina"'
Autor:
Rossi, Martina, Romano, Donatella, Mucciarelli, Alessio, Ceccarelli, Edoardo, Massari, Davide, Zamorani, Giovanni
Context. The recent detection of nitrogen-enhanced, metal-poor galaxies at high redshift by the James Webb Space Telescope has sparked renewed interest in exploring the chemical evolution of carbon, nitrogen, and oxygen (the CNO elements) at early ti
Externí odkaz:
http://arxiv.org/abs/2406.14615
The elusive properties of the first (Pop III) stars can be indirectly unveiled by uncovering their true descendants. To this aim, we exploit our data-calibrated model for the best-studied ultra-faint dwarf (UFD) galaxy, Bo\"otes I, which tracks the c
Externí odkaz:
http://arxiv.org/abs/2406.12960
The metal-poor stars in the Galactic halo are thought to show the imprints of the first (PopIII) stars, and thus provide a glance at the first episodes of star formation. In this work, we aim at understanding whether all very metal-poor stars formed
Externí odkaz:
http://arxiv.org/abs/2309.07958
Autor:
Rossi, Martina
Publikováno v:
Venezia Arti, Vol 26, Iss 1, Pp - (2017)
Pino Pascali’s Requiescat in Pace Corradinus is a happening that took place on 22nd July 1965 in the castle of Torre Astura, in the frame of an exhibition promoted by La Salita gallery (Rome). The artist performed a funeral rite in a crypt, in fron
Externí odkaz:
https://doaj.org/article/aa6eec4a6ecf46debd69670b0a6af40a
Autor:
Bonaldi, Nicolò, Rossi, Martina, Mattioli, Daniele, Grapulin, Michele, Fernández, Blanca Silva, Caputo, Davide, Magagnini, Marco, Osti, Arianna, Veronese, Fabio
Gaussian Boson Sampling (GBS) is a recently developed paradigm of quantum computing consisting of sending a Gaussian state through a linear interferometer and then counting the number of photons in each output mode. When the system encodes a symmetri
Externí odkaz:
http://arxiv.org/abs/2307.13348
Autor:
Pagnini, Giulia, Salvadori, Stefania, Rossi, Martina, Aguado, David, Koutsouridou, Ioanna, Skúladóttir, Ása
The chemical fingerprints of the first stars are retained within the photospheres of ancient unevolved metal-poor stars. A significant fraction of these stellar fossils is represented by stars known as Carbon-Enhanced Metal-Poor (CEMP), $\rm [C/Fe]>+
Externí odkaz:
http://arxiv.org/abs/2303.14204
This book aims at encompassing the panorama of design tools being developed, tested and adopted by researchers and professors at the Department of Design of Politecnico di Milano. The tools are organized in a taxonomy that reflects the path of choice
Externí odkaz:
https://library.oapen.org/handle/20.500.12657/57701
The origin of Carbon Enhanced Metal-Poor (CEMP-no) stars with low abundances of neutron-capture elements is still unclear. These stars are ubiquitous, found primarily in the Milky Way halo and ultra-faint dwarf galaxies (UFDs). To make a major step f
Externí odkaz:
http://arxiv.org/abs/2302.10210
Autor:
Sallustio, Valentina, Rossi, Martina, Marto, Joana, Coelho, Tiago, Chinnici, Fabio, Mandrone, Manuela, Chiocchio, Ilaria, Cappadone, Concettina, Luppi, Barbara, Bigucci, Federica, Abruzzo, Angela, Cerchiara, Teresa
Publikováno v:
In Industrial Crops & Products 15 October 2024 218