Zobrazeno 1 - 10
of 194
pro vyhledávání: '"Inno, L"'
Autor:
da Silva, R., D'Orazi, V., Palla, M., Bono, G., Braga, V. F., Fabrizio, M., Lemasle, B., Spitoni, E., Matteucci, F., Jonsson, H., Kovtyukh, V., Magrini, L., Bergemann, M., Dall'Ora, M., Ferraro, I., Fiorentino, G., Francois, P., Iannicola, G., Inno, L., Kudritzki, R. -P., Matsunaga, N., Monelli, M., Nonino, M., Sneden, C., Storm, J., Thevenin, F., Tsujimoto, T., Zocchi, A.
Publikováno v:
A&A 678, A195 (2023)
Classical Cepheids (CCs) are solid distance indicators and tracers of young stellar populations. Our aim is to provide iron, oxygen, and sulfur abundances for the largest and most homogeneous sample of Galactic CCs ever analyzed. The current sample c
Externí odkaz:
http://arxiv.org/abs/2308.01928
Autor:
da Silva, R., Crestani, J., Bono, G., Braga, V. F., D'Orazi, V., Lemasle, B., Bergemann, M., Dall'Ora, M., Fiorentino, G., François, P., Groenewegen, M. A. T., Inno, L., Kovtyukh, V., Kudritzki, R. -P., Matsunaga, N., Monelli, M., Pietrinferni, A., Porcelli, L., Storm, J., Tantalo, M., Thévénin, F.
Publikováno v:
A&A 661, A104 (2022)
Classical Cepheids are the most popular distance indicators and tracers of young stellar populations. The key advantage is that they are bright and they can be easily identified in Local Group and Local Volume galaxies. Their evolutionary and pulsati
Externí odkaz:
http://arxiv.org/abs/2202.07945
Autor:
Polimeno, P., Magazzu, A., Iati, M. A., Saija, R., Folco, L., Ciriza, D. Bronte, Donato, M. G., Foti, A., Gucciardi, P. G., Saidi, A., Cecchi-Pestellini, C., Escobar, A. Jimenez, Ammannito, E., Sindoni, G., Bertini, I., Della Corte, V., Inno, L., Ciaravella, A., Rotundi, A., Marago, O. M.
Publikováno v:
Eur. Phys. J. Plus (2021) 136:339
Optical tweezers are powerful tools based on focused laser beams. They are able to trap, manipulate and investigate a wide range of microscopic and nanoscopic particles in different media, such as liquids, air, and vacuum. Key applications of this co
Externí odkaz:
http://arxiv.org/abs/2111.06397
Autor:
Braga, V. F., Crestani, J., Fabrizio, M., Bono, G., Preston, G. W., Sneden, C., Storm, J., Kamann, S., Latour, M., Lala, H., Lemasle, B., Prudil, Z., Altavilla, G., Chaboyer, B., Dall'Ora, M., Ferraro, I., Gilligan, C. K., Fiorentino, G., Iannicola, G., Inno, L., Kwak, S., Marengo, M., Marinoni, S., Marrese, P. M., Martínez-Vázquez, C. E., Monelli, M., Mullen, J. P., Matsunaga, N., Neeley, J., Stetson, P. B., Valenti, E., Zoccali, M.
We collected the largest spectroscopic catalog of RR Lyrae (RRLs) including $\approx$20,000 high-, medium- and low-resolution spectra for $\approx$10,000 RRLs. We provide the analytical forms of radial velocity curve (RVC) templates. These were built
Externí odkaz:
http://arxiv.org/abs/2107.00923
Autor:
Magrini, L., Lagarde, N., Charbonnel, C., Franciosini, E., Randich, S., Smiljanic, R., Casali, G., Vazquez, C. Viscasillas, Spina, L., Biazzo, K., Pasquini, L., Bragaglia, A., Van der Swaelmen, M., Tautvaisiene, G., Inno, L., Sanna, N., Prisinzano, L., Degl'Innocenti, S., Moroni, P. Prada, Roccatagliata, V., Tognelli, E., Monaco, L., de Laverny, P., Delgado-Mena, E., Baratella, M., D'Orazi, V., Vallenari, A., Gonneau, A., Worley, C., Jimenez-Esteban, F., Jofre, P., Bensby, T., Francois, P., Guiglion, G., Bayo, A., Jeffries, R. D., Binks, A. S., Korn, A., Gilmore, G., Damiani, F., Pancino, E., Sacco, G. G., Hourihane, A., Morbidelli, L., Zaggia, S.
Publikováno v:
A&A 651, A84 (2021)
We aim to constrain the mixing processes in low-mass stars by investigating the behaviour of the Li surface abundance after the main sequence. We take advantage of the data from the sixth internal data release of Gaia-ESO, idr6, and from the Gaia Ear
Externí odkaz:
http://arxiv.org/abs/2105.04866
We present a well-defined and characterized all-sky sample of classical Cepheids in the Milky Way, obtained by combining two time-domain all-sky surveys: Gaia DR2 (Gaia Collaboration et al. 2018) and ASAS-SN (Shappee et al. 2014). We first use parall
Externí odkaz:
http://arxiv.org/abs/2103.08597
Autor:
Crestani, J., Fabrizio, M., Braga, V. F., Sneden, C., Preston, G. W., Ferraro, I., Iannicola, G., Bono, G., Alves-Brito, A., Nonino, M., D'Orazi, V., Inno, L., Monelli, M., Storm, J., Altavilla, G., Chaboyer, B., Dall'Ora, M., Fiorentino, G., Gilligan, C. K., Grebel, E., Lala, H., Lemasle, B., Marengo, M., Marinoni, S., Marrese, P. M., Martínez-Vázquez, C. E., Matsunaga, N., Mullen, J. P., Neeley, J., Prudil, Z., da Silva, R., Stetson, P. B., Thévenin, F., Valenti, E., Walker, A. R., Zoccali, M.
We performed the largest and most homogeneous spectroscopic survey of field RR Lyraes (RRLs). We secured $\approx$6,300 high resolution (HR, R$\sim$35,000) spectra for 143 RRLs (111 fundamental, RRab; 32 first overtone, RRc). The atmospheric paramete
Externí odkaz:
http://arxiv.org/abs/2012.02284
Autor:
Bono, G., Braga, V. F., Crestani, J., Fabrizio, M., Sneden, C., Marconi, M., Preston, G. W., Mullen, J. P., Gilligan, C. K., Fiorentino, G., Pietrinferni, A., Altavilla, G., Buonanno, R., Chaboyer, B., da Silva, R., Dall'Ora, M., Degl'Innocenti, S., Di Carlo, E., Ferraro, I., Grebel, E., Iannicola, G., Inno, L., Kovtyukh, V., Kunder, A., Lemasle, B., Marengo, M., Marinoni, S., Marrese, P. M., Martínez-Vázquez, C. E., Matsunaga, N., Monelli, M., Neeley, J., Nonino, M., Moroni, P. G. Prada, Prudil, Z., Stetson, P. B., Thévenin, F., Tognelli, E., Valenti, E., Walker, A. R.
We collected over 6000 high-resolution spectra of four dozen field RR Lyrae (RRL) variables pulsating either in the fundamental (39 RRab) or in the first overtone (9 RRc) mode. We measured radial velocities (RVs) of four strong metallic and four Balm
Externí odkaz:
http://arxiv.org/abs/2005.11566
Autor:
Magurno, D., Sneden, C., Bono, G., Braga, V. F., Mateo, M., Persson, S. E., Preston, G., Thevenin, F., da Silva, R., Dall'Ora, M., Fabrizio, M., Ferraro, I., Fiorentino, G., Iannicola, G., Inno, L., Marengo, M., Marinoni, S., Marrese, P. M., Martinez-Vazquez, C. E., Matsunaga, N., Monelli, M., Neeley, J. R., Nonino, M., Walker, A. R.
We present a detailed spectroscopic analysis of RR Lyrae (RRL) variables in the globular cluster NGC 5139 (omega Cen). We collected optical (4580-5330 A), high resolution (R = 34,000), high signal-to-noise ratio (200) spectra for 113 RRLs with the mu
Externí odkaz:
http://arxiv.org/abs/1906.08550
Autor:
Della Corte, V., Ferretti, S., Piccirillo, A.M., Zakharov, V., Di Paolo, F., Rotundi, A., Ammannito, E., Amoroso, M., Bertini, I., Di Donato, P., Ferraioli, G., Fiscale, S., Fulle, M., Inno, L., Longobardo, A., Mazzotta-Epifani, E., Muscari Tomajoli, M.T., Sindoni, G., Tonietti, L., Rothkaehl, H., Wozniakiewicz, P.J., Burchell, M.J., Alesbrook, L.A., Sylvest, M.E., Patel, M.R.
Publikováno v:
In Advances in Space Research 15 April 2023 71(8):3457-3467
