Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Marco Tailo"'
Autor:
Giacomo Cordoni, Antonino P. Milone, Anna F. Marino, Michele Cignoni, Edoardo P. Lagioia, Marco Tailo, Marília Carlos, Emanuele Dondoglio, Sohee Jang, Anjana Mohandasan, Maria V. Legnardi
Publikováno v:
Nature Communications, Vol 13, Iss 1, Pp 1-9 (2022)
The nature of young star clusters in the Magellanic Clouds is debated. Here, the authors show an alternative approach that exploits data to exclude the presence of age differences greater than a few million years among cluster stars in a very young c
Externí odkaz:
https://doaj.org/article/89b418e3a30c4e89b8e8913230a26f86
Autor:
Paolo Ventura, Flavia Dell’Agli, Marco Tailo, Marco Castellani, Ester Marini, Silvia Tosi, Marcella Di Criscienzo
Publikováno v:
Universe, Vol 8, Iss 1, p 45 (2022)
We discuss the evolution of stars through the asymptotic giant branch, focusing on the physical mechanisms potentially able to alter the surface chemical composition and on how changes in the chemistry of the external regions affect the physical prop
Externí odkaz:
https://doaj.org/article/bbf7154d7a4240e5b1dbaf7c890751ab
Autor:
Marco Tailo
Publikováno v:
Proceedings of the International Astronomical Union. 16:321-326
The amount of mass lost by stars during the red-giant branch (RGB) phase is one of the main parameters needed to fully understand later stages of stellar evolution. In spite of its importance, a fully-comprehensive physical understanding of this phen
Autor:
Francesca D’Antona, Marco Tailo
Publikováno v:
Astrophysics and Space Science Library ISBN: 9783030851972
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4f5242f97d7de36c22041181a84bb337
https://doi.org/10.1007/978-3-030-85198-9_7
https://doi.org/10.1007/978-3-030-85198-9_7
Autor:
Marcella Di Criscienzo, Andrea Bellini, Paolo Ventura, Marco Tailo, Thibaut Decressin, Roberto Capuzzo-Dolcetta, V. Caloi, Enrico Vesperini, Aaron Dotter, Francesca D'Antona, Annibale D'Ercole, Antonino Milone
Publikováno v:
Nature. 523:318-321
Horizontal Branch stars belong to an advanced stage in the evolution of the oldest stellar galactic population, occurring either as field halo stars or grouped in globular clusters. The discovery of multiple populations in these clusters, that were p
Publikováno v:
Astronomical Journal; Nov2019, Vol. 158 Issue 5, p1-1, 1p
Autor:
Francesca D’Antona, Paolo Ventura, Anna Fabiola Marino, Antonino P. Milone, Marco Tailo, Marcella Di Criscienzo, Enrico Vesperini
Publikováno v:
Astrophysical Journal Letters; 1/20/2019, Vol. 871 Issue 1, p1-1, 1p
Autor:
Marco, Tailo, Milone, Antonino P., Lagioia, Edoardo P., D'Antona, Francesca, Sohee Jang, Vesperini, Enrico, Marino, Anna F., Ventura, Paolo, Caloi, Vittoria, Marilia Carlos, Cordoni, Giacomo, Dondoglio, Emanuele, Mohandasan, Anjana, J. Ephrem Nastasio, Legnardi, Maria Vittoria
Poster for the Cool stars 20.5 virtual conference. Abstract: The amount of mass lost by stars during the red-giant branch (RGB) phase is one of the main parameters to correctly study later stages of stellar evolution. In spite of its importance, a fu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8c680546f5951b1b0f5088ee1314cad1
Publikováno v:
Proceedings of the International Astronomical Union. Nov2022, Vol. 16 Issue S366, pf1-f23. 23p.
Autor:
Tailo, Marco1 mrctailo@gmail.com
Publikováno v:
Proceedings of the International Astronomical Union. Nov2022, Vol. 16 Issue S366, p321-326. 6p.