Zobrazeno 1 - 10
of 579
pro vyhledávání: '"Pecci F"'
Autor:
Di Federico, A., Alden, S.L., Smithy, J.W., Ricciuti, B., Alessi, J.V., Wang, X., Pecci, F., Lamberti, G., Gandhi, M.M., Vaz, V.R., Spurr, L.F., Sholl, L.M., Pfaff, K.L., Rodig, S.J., Li, Y.Y., Cherniack, A.D., Nishino, M., Johnson, B.E., Awad, M.M.
Publikováno v:
In Annals of Oncology
Autor:
Cantini, L., Mentrasti, G., Russo, G.L., Signorelli, D., Pasello, G., Rijavec, E., Russano, M., Antonuzzo, L., Rocco, D., Giusti, R., Adamo, V., Genova, C., Tuzi, A., Morabito, A., Gori, S., Verde, N. La, Chiari, R., Cortellini, A., Cognigni, V., Pecci, F., Indini, A., De Toma, A., Zattarin, E., Oresti, S., Pizzutilo, E.G., Frega, S., Erbetta, E., Galletti, A., Citarella, F., Fancelli, S., Caliman, E., Della Gravara, L., Malapelle, U., Filetti, M., Piras, M., Toscano, G., Zullo, L., De Tursi, M., Di Marino, P., D’Emilio, V., Cona, M.S., Guida, A., Caglio, A., Salerno, F., Spinelli, G., Bennati, C., Morgillo, F., Russo, A., Dellepiane, C., Vallini, I., Sforza, V., Inno, A., Rastelli, F., Tassi, V., Nicolardi, L., Pensieri, V., Emili, R., Roca, E., Migliore, A., Galassi, T., Rocchi, M. L. Bruno, Berardi, R.
Publikováno v:
In ESMO Open April 2022 7(2)
Autor:
Origlia, L., Ferraro, F. R., Fabbri, S., Pecci, F. Fusi, Dalessandro, E., Rich, R. M., Valenti, E.
The main aim of the present work is to derive an empirical mass-loss (ML) law for Population II stars in first and second ascent red giant branches. We used the Spitzer InfraRed Array Camera (IRAC) photometry obtained in the 3.6-8 micron range of a c
Externí odkaz:
http://arxiv.org/abs/1403.4096
Autor:
Bellazzini, M., Buzzoni, A., Cacciari, C., Federici, L., Pecci, F. Fusi, Galleti, S., Perina, S.
We present the results of a first global analysis of the Horizontal Branch morphology of Globular Clusters in the nearby spiral M31, based on their Color Magnitude Diagrams.
Comment: 4 pages, 3 figures, proceedings of the meeting "Reading the bo
Comment: 4 pages, 3 figures, proceedings of the meeting "Reading the bo
Externí odkaz:
http://arxiv.org/abs/1301.3306
Autor:
Perina, S., Bellazzini, M., Buzzoni, A., Cacciari, C., Federici, L., Pecci, F. Fusi, Galleti, S.
We use deep, high quality colour magnitude diagrams obtained with the Hubble Space Telescope to compute a simplified version of the Mironov index [SMI; B/(B+R)] to parametrize the horizontal branch (HB) morphology for 23 globular clusters in the M31
Externí odkaz:
http://arxiv.org/abs/1209.2130
Autor:
Pancino, E., Altavilla, G., Marinoni, S., Cocozza, G., Carrasco, J. M., Bellazzini, M., Bragaglia, A., Federici, L., Rossetti, E., Cacciari, C., Nunez, L. Balaguer, Castro, A., Figueras, F., Pecci, F. Fusi, Galleti, S., Gebran, M., Jordi, C., Lardo, C., Masana, E., Monguio, M., Montegriffo, P., Ragaini, S., Schuster, W., Trager, S., Vilardell, F., Voss, H.
We describe two ground based observing campaigns aimed at building a grid of approximately 200 spectrophotometric standard stars (SPSS), with an internal ~1% precision and tied to Vega within ~3%, for the absolute flux calibration of data gathered by
Externí odkaz:
http://arxiv.org/abs/1207.6042
We present deep (V ~ 28.0) BV photometry obtained with the wide field channel of the Advanced Camera for Surveys on board HST for four M31 globular clusters that were identified as candidate intermediate-age (age ~ 1-9 Gyr) by various authors, based
Externí odkaz:
http://arxiv.org/abs/1106.1431
Autor:
Dalessandro, E., Salaris, M., Ferraro, F. R., Cassisi, S., Lanzoni, B., Rood, R. T., Pecci, F. Fusi, Sabbi, E.
We present an accurate analysis of the peculiar Horizontal Branch (HB) of the massive Galactic globular cluster NGC 2808, based on high-resolution far-UV and optical images of the central region of the cluster obtained with HST. We confirm the multim
Externí odkaz:
http://arxiv.org/abs/1008.4478
Autor:
Lovisi, L., Mucciarelli, A., Ferraro, F. R., Lucatello, S., Lanzoni, B., Dalessandro, E., Beccari, G., Rood, R. T., Sills, A., Pecci, F. Fusi, Gratton, R., Piotto, G.
We have used high resolution spectra obtained with the spectrograph FLAMES at the ESO Very Large Telescope to determine the kinematical properties and the abundance patterns of 20 blue straggler stars (BSSs) in the globular cluster M4. We found that
Externí odkaz:
http://arxiv.org/abs/1007.2343
We have investigated the relevant trend of the bolometric correction (BC) at the cool-temperature regime of red giant stars and its possible dependence on stellar metallicity. Our analysis relies on a wide sample of optical-infrared spectroscopic obs
Externí odkaz:
http://arxiv.org/abs/1002.1972