Zobrazeno 1 - 10
of 196
pro vyhledávání: '"F R, Ferraro"'
Publikováno v:
The Astrophysical Journal, Vol 968, Iss 1, p 2 (2024)
We recently introduced three new parameters that describe the shape of the normalized cumulative radial distribution (nCRD) of the innermost stars in globular clusters (GCs) and trace the clusters’ dynamical evolution. Here, we extend our previous
Externí odkaz:
https://doaj.org/article/94275d2dc56c4ddab59a3ac3235df5e3
Publikováno v:
The Astrophysical Journal, Vol 945, Iss 2, p 164 (2023)
By studying the normalized cumulative radial distribution (nCRD) of the stars in the central region of a Monte Carlo-simulated globular cluster, we recently defined three parameters able to pinpoint the stage of internal dynamical evolution reached b
Externí odkaz:
https://doaj.org/article/e35db68d46614ed291c1dcc5e3daf952
We present a numerical study, based on Monte Carlo simulations, aimed at defining new empirical parameters measurable from observations and able to trace the different phases of star cluster dynamical evolution. As expected, a central density cusp, d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::90b95b767b1e110c5238c2c4d3891cf1
https://hdl.handle.net/11585/902054
https://hdl.handle.net/11585/902054
Autor:
F. R. Ferraro
Publikováno v:
The Wiley Encyclopedia of Personality and Individual Differences
Autor:
F. R. Ferraro
Publikováno v:
The Wiley Encyclopedia of Personality and Individual Differences. :483-486
Publikováno v:
Current Psychology. 41:2980-2984
Two studies had undergraduates (n = 237) walk a path in a university building which included walking up a set of stairs, through two hallways and walking down a flight of stairs back to the research lab. Subjects responded to text messages with a sin
Autor:
F. Dresbach, D. Massari, B. Lanzoni, F. R. Ferraro, E. Dalessandro, S. Raso, A. Bellini, M. Libralato
Publikováno v:
Astrophysical Journal, 928(1):47. IOP PUBLISHING LTD
The level of central segregation of Blue Straggler stars proved to be an excellent tracer of the dynamical evolution of old star clusters (the so-called "dynamical clock"), both in the Milky Way and in the Large Magellanic Cloud. The $A^{+}$ paramete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f15367ceeab3b00262575152a844d15e
https://research.rug.nl/en/publications/ff59aefe-ea6e-4a18-9d5e-e6d127b2f127
https://research.rug.nl/en/publications/ff59aefe-ea6e-4a18-9d5e-e6d127b2f127
Publikováno v:
Astronomy & Astrophysics. 671:A124
We present the chemical composition of 206 red giant branch stars members of the Small Magellanic Cloud (SMC) using optical, high-resolution spectra collected with the multi-object spectrograph FLAMES-GIRAFFE at the ESO Very Large Telescope. This sam
Autor:
Rosanna Depalo, A. Best, Antonio Caciolli, K. Stöckel, I. Kochanek, Davide Trezzi, Gianluca Imbriani, R. Perrino, E. Masha, Luigi Schiavulli, F. R. Ferraro, M. P. Takács, V. Paticchio, A. Formicola, F. R. Pantaleo, Francesco Barile, T. Chillery, T. Davinson, Daniel Bemmerer, G. F. Ciani, Tamás Szücs, A. Guglielmetti, László Csedreki, D. Rapagnani, Oscar Straniero, A. Di Leva, Sandra Zavatarelli, Gy. Gyürky, Michael Wiescher, G. Gervino, A. Boeltzig, Zs. Fülöp, V. Mossa, Marialuisa Aliotta, J. Balibrea-Correa, Carlo Bruno, E. M. Fiore, M. Junker, C. Gustavino, G. D'Erasmo, F. Cavanna, Paolo Prati, Carlo Broggini, M. Lugaro, Raffaele Buompane, Richard deBoer, R. Menegazzo, D. Piatti, Z. Elekes, P. Corvisiero
Publikováno v:
Physical Review C. 104
Background: Shell hydrogen burning during the asymptotic giant branch (AGB) phase through the oxygen isotopes has been indicated as a key process that is needed to understand the observed O 18 / O 16 relative abundance in presolar grains and in stell
Autor:
Gianluca Imbriani, A. Boeltzig, A. Gnech, V. Mossa, T. Davinson, Carlo Bruno, R. Menegazzo, Laura Elisa Marcucci, G. F. Ciani, M. P. Takács, Antonio Caciolli, Oscar Straniero, F. Cavanna, Gy. Gyürky, M. Junker, Marialuisa Aliotta, Rosanna Depalo, A. Best, T. Chillery, Z. Elekes, C. Gustavino, E. Masha, A. Di Leva, Luigi Schiavulli, G. Gervino, P. Corvisiero, V. Paticchio, A. Formicola, Zs. Fülöp, K. Stöckel, Paolo Prati, M. Lugaro, D. Piatti, A. Guglielmetti, László Csedreki, F. R. Pantaleo, Carlo Broggini, I. Kochanek, Sandra Zavatarelli, Paola Marigo, Daniel Bemmerer, R. Perrino, F. R. Ferraro, Tamás Szücs, E. M. Fiore
Publikováno v:
Physical Review C. 102