Zobrazeno 1 - 10
of 14 916
pro vyhledávání: '"A Milone"'
Autor:
Muratore, F., Milone, A. P., D'Antona, F., Nastasio, E. J., Cordoni, G., Legnardi, M. V., He, C., Ziliotto, T., Dondoglio, E., Bernizzoni, M., Tailo, M., Bortolan, E., Dell'Agli, F., Deng, L., Lagioia, E. P., Li, C., Marino, A. F., Ventura, P.
Nearly all star clusters younger than ~600 Myr exhibit extended main sequence turn offs and split main sequences (MSs) in their color-magnitude diagrams. Works based on both photometry and spectroscopy have firmly demonstrated that the red MS is comp
Externí odkaz:
http://arxiv.org/abs/2411.02508
Inspired by the success of large language models (LLM) for DNA and proteins, several LLM for RNA have been developed recently. RNA-LLM uses large datasets of RNA sequences to learn, in a self-supervised way, how to represent each RNA base with a sema
Externí odkaz:
http://arxiv.org/abs/2410.16212
Autor:
Cordoni, Giacomo, Casagrande, Luca, Milone, Antonino, Dondoglio, Emanuele, Mastrobuono-Battisti, Alessandra, Jang, Sohee, Marino, Anna, Lagioia, Edoardo, Legnardi, Maria Vittoria, Ziliotto, Tuila, Muratore, Fabrizio, Mehta, Vernica, Lacchin, Elena, Tailo, Marco
We present the first comprehensive analysis of the internal dynamics of multiple stellar populations (MPs) in 28 Galactic Globular Clusters (GCs) across a wide field of view, extending from the innermost regions to the clusters' outskirts. Using astr
Externí odkaz:
http://arxiv.org/abs/2409.02330
Publikováno v:
Lupus Science and Medicine, Vol 9, Iss Suppl 2 (2022)
Externí odkaz:
https://doaj.org/article/e415e58350d44a40ba7855a682e7f4c4
Autor:
S Fasano, R Tirri, F Ciccia, F Riccio, A Milone, M Patrone, L Sadile, M Fabrazzo, E Di Caprio
Publikováno v:
Lupus Science and Medicine, Vol 9, Iss Suppl 2 (2022)
Externí odkaz:
https://doaj.org/article/fab49cf5802b4dffb730b1b6ff6ab7a5
Autor:
Cordoni, Giacomo, Casagrande, Luca, Yu, Jie, Milone, Antonino P., Marino, Anna F., D'Antona, Francesca, Dell'Agli, Flavia, Buder, Sven, Tailo, Marco
The origin of extended main-sequence turn-offs (eMSTO) in star clusters younger than 2 Gyr still challenges our current understanding of stellar evolution. Exploiting data from Gaia Data Release 3 (DR3), we investigate eMSTOs in a large sample of 32
Externí odkaz:
http://arxiv.org/abs/2406.16551
Autor:
Lagioia, E. P., Milone, A. P., Legnardi, M. V., Cordoni, G., Dondoglio, E., Renzini, A., Tailo, M., Ziliotto, T., Carlos, M., Jang, S., Marino, A. F., Mohandasan, A., Qi, J., Rangwal, G., Bortolan, E., Muratore, F.
The pseudo two-color diagram, known as chromosome map (ChM), is a valuable tool for identifying globular clusters (GCs) that consist of single or multiple stellar populations (MPs). Recent surveys of Galactic GCs using the ChM have provided stringent
Externí odkaz:
http://arxiv.org/abs/2406.16824
Autor:
Marino, A. F., Milone, A. P., Renzini, A., Dondoglio, E., Bortolan, E., Carlos, M. G., Cordoni, G., Dotter, A., Jang, S., Lagioia, E. P., Legnardi, M. V., Muratore, F., Mohandasan, A., Tailo, M., Ziliotto, T.
We present the first spectroscopic estimates of the chemical abundance of M dwarf stars in a globular cluster (GC), namely 47 Tucanae. By exploiting NIRSpec on board the James Webb Space Telescope (JWST) we gathered low-resolution spectra for 28 star
Externí odkaz:
http://arxiv.org/abs/2406.12684
Autor:
Cristofari, Paul I., Dupree, Andrea K., Milone, Antonino P., Walker, Matthew G., Mateo, Mario, Dotter, Aaron, Bailey III, John I.
We present an analysis of high-resolution optical spectra recorded for 30 stars of the split extended main-sequence turnoff (eMSTO) of the young ($\sim$ 40 Myr) Small Magellanic Cloud (SMC) globular cluster NGC 330. Spectra were obtained with the M2F
Externí odkaz:
http://arxiv.org/abs/2406.10413
Autor:
Mehta, V. J., Milone, A. P., Casagrande, L., Marino, A. F., Legnardi, M. V., Cordoni, G., Dondoglio, E., Jang, S., Ziliotto, T., Barbieri, M., Bernizzoni, M., Bortolan, E., Sanchez, A. Bouras Moreno, Lagioia, E. P., Lionetto, S., Mohandasan, A., Muratore, F.
Understanding the formation of multiple populations in globular clusters (GCs) represents a challenge for stellar population studies. Nevertheless, the outermost cluster regions, likely to hold clues about the initial configuration of GC stars, remai
Externí odkaz:
http://arxiv.org/abs/2406.02755