Results 81 to 90 of about 41,067 (162)
Multiple populations in globular clusters. Lessons learned from the
Milky Way globular clusters
, 2012 Recent progress in studies of globular clusters has shown that they are not
simple stellar populations, being rather made of multiple generations. Evidence
stems both from photometry and spectroscopy.A Bellini, A Bragaglia, A Bragaglia, A Buzzoni, A Dotter, A Duquennoy, A D’Ercole, A D’Ercole, A Helmi, A Helmi, A Kayser, A Klypin, A Koch, A Korn, A Krabbe, A Maeder, A Marino, A McWilliam, A Moretti, A Mucciarelli, A Mucciarelli, A Recio-Blanco, A Renzini, A Sandage, A Sarajedini, A Siebert, A Sollima, A Sollima, AA Kepley, AAR Valcarce, AC Boley, AD Mackey, AF Marino, AF Marino, AF Marino, AF Marino, AGW Cameron, AI Karakas, AK Dupree, Angela Bragaglia, AP Milone, AP Milone, AP Milone, AP Milone, AR Walker, AV Kravtsov, AV Macciò, AV Sweigart, AV Sweigart, B Davies, B Davies, B Gao, B Letarte, B Moore, B Yanny, BB Behr, BB Behr, BG Elmegreen, BJ Anthony-Twarog, BJ Armosky, BW Carney, C Chiappini, C Conroy, C Lardo, C Sneden, C Sneden, C Sneden, C Sosin, CA Pilachowski, CB Stephenson, CF McKee, CI Johnson, CI Johnson, CJ Grillmair, CJ Lada, CJ Walcher, D Butler, D Carollo, D Fabbian, D Harbeck, D Heggie, D Schaerer, D Yong, D Yong, D Yong, D Yong, D Yong, D Yong, D Yong, D Yong, D-G Roh, DA Crocker, DC Heggie, DE McLaughlin, DE McLaughlin, DK Lai, E Bica, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Carretta, E Hennekemper, E Pancino, E Pancino, E Pancino, E Tolstoy, E Vesperini, E Vesperini, E Vesperini, EA Mallia, EN Kirby, Eugenio Carretta, EW Olszewski, F Caputo, F D’Antona, F D’Antona, F D’Antona, F D’Antona, F D’Antona, F D’Antona, F D’Antona, F D’Antona, F D’Antona, F Fusi Pecci, F Grundahl, FR Ferraro, FR Ferraro, FR Ferraro, FR Ferraro, G Bertelli, G James, G Marchi De, G Marchi De, G Michaud, G Pace, G Parmentier, G Parmentier, G Piotto, G Piotto, G Piotto, G Piotto, G Schaller, G Tenorio-Tagle, G Zhao, GE Langer, GH Smith, GH Smith, GH Smith, GH Smith, GM Silva de, GS Costa Da, H Baumgardt, HB Richer, HJGLM Lamers, HL Morrison, I Negueruela, I-J Sackmann, II Ivans, II Ivans, IU Roederer, IU Roederer, J Anderson, J Dabringhausen, J Goodman, J Greissl, J Norris, J Pflamm-Altenburg, J Rossa, J Vinkó, J-W Lee, JA Johnson, JE Hesser, JE Norris, JE Norris, JG Cohen, JG Cohen, JG Cohen, JG Cohen, JG Cohen, JG Cohen, JG Cohen, JG Cohen, JL Greenstein, JM Scalo, JMD Kruijssen, JP Brodie, JR Hurley, JS Bullock, JW Truran, K Bekki, K Bekki, K Bekki, K Bekki, K Bekki, K Bekki, K Bekki, K Freeman, K Freeman, K Glatt, K Jordi, K Lind, K Lind, KC Freeman, L Aguilar, L Girardi, L Greggio, L Origlia, L Pasquini, L Pasquini, L Sbordone, L Siess, LM Stanford, LM Stanford, LR Bedin, M Arnould, M Bellazzini, M Catelan, M Catelan, M Criscienzo di, M Criscienzo di, M Gieles, M Henon, M Hilker, M Jurić, M Odenkirchen, M Odenkirchen, M Ricotti, M Salaris, M Shetrone, M Steinmetz, M Steinmetz, M Trenti, M Wadepuhl, M Zoccali, MAC Perryman, MF Nieva, MH Siegel, MM Briley, MM Briley, MM Briley, MM Briley, N Bastian, N Ivanova, N Ivanova, N Prantzos, N Prantzos, OY Gnedin, P Bonifacio, P Goudfrooij, P Ventura, P Ventura, P Ventura, P Ventura, P Ventura, P Ventura, P Ventura, P Ventura, PA Denisenkov, PL Cottrell, R Gilmozzi, R Gratton, R Gratton, R Gratton, Raffaele G. Gratton, RC Brüns, RC Peterson, RD Cannon, RG Gratton, RG Gratton, RG Gratton, RG Gratton, RG Gratton, RG Gratton, RG Gratton, RG Gratton, RI Thompson, RK Bhatia, RM Cavallo, RM Rich, RP Kraft, RP Kraft, RP Kraft, RP Kraft, RW Romani, S Bergh van den, S Bergh van den, S Cassisi, S Moehler, S Moehler, S Rubele, S Villanova, S Villanova, S Villanova, S-H Chun, S-I Han, SA Becker, SC Keller, SDM White, SE Mink de, SF Portegies Zwart, SG Ryan, SL Martell, SL Martell, SL Martell, SM Fall, SM Fall, SP Goodwin, SV Ramírez, SV Ramírez, SW Campbell, SW Campbell, T Bloecker, T Böker, T Böker, T Decressin, T Decressin, T Decressin, T Decressin, T Decressin, TC Beers, TD Kinman, V Belokurov, V Caloi, V Caloi, V Caloi, V Caloi, V D’Orazi, V D’Orazi, V D’Orazi, V D’Orazi, V D’Orazi, V Kravtsov, V Kravtsov, VV Smith, W Osborn, WE Harris, WE Harris, WE Harris, WR Brown, Y-W Lee, Y-W Lee, Y-W Lee, Z-X Shen, Z-X Shen, Ž Ivezić +359 morecore +1 more sourceThe Distance of the First Overtone RR Lyrae Variables in the MACHO LMC
Database: A New Method to Correct for the Effects of Crowding
, 2007 Previous studies have indicated that many of the RR Lyrae variables in the
LMC have properties similar to the ones in the Galactic globular cluster M3.A. V. Muzzin, Bailey S. I., C. M. Clement, Cacciari C., Cacciari C., Castelli F., Castelli F., Catelan M., Clement C. M., Longmore A. J., Schwering P. B. W. & Israel F. P., Szeidl B., X. Xu +12 morecore +1 more sourceThe origin of the spurious iron spread in the globular cluster NGC 3201
, 2015 NGC 3201 is a globular cluster suspected to have an intrinsic spread in the
iron content. We re-analysed a sample of 21 cluster stars observed with
UVES-FLAMES at the Very Large Telescope and for which Simmerer et al.Ferraro, F. R., Lanzoni, B., Lapenna, E., Massari, D., Mucciarelli, A. +4 morecore +1 more sourceChemical and kinematical properties of BSSs and HB stars in NGC 6397
, 2012 We used three sets of high-resolution spectra acquired with the multifiber
facility FLAMES at the Very Large Telescope of the European Southern
Observatory to investigate the chemical and kinematical properties of a sample
of 42 horizontal branch (HB ...A. Mucciarelli, B. Lanzoni, Behr, Behr, Behr, Behr, Carretta, Carretta, Castelli, Castelli, Castelli, De Marco, D’Antona, E. Dalessandro, F. R. Ferraro, Ferraro, Ferraro, For, González Hernández, Gratton, Grundahl, Hills, Johnson, Kaluzny, Kurucz, L. Lovisi, Leonard, Lovisi, Marino, McCrea, Michaud, Moehler, Mucciarelli, Origlia, Peterson, Pietrinferni, R. Contreras Ramos, R. Gratton, Recio-Blanco, Richard, Sarna, Sbordone, Shara, Sills, Takeda, Varenne, Vauclair +46 morecore +1 more sourceHelium in first and second-generation stars in Globular Clusters from
spectroscopy of red giants
, 2010 (abridged) Recent spectroscopic and photometric observations show the
existence of various generations of stars in GCs, differing in the abundances
of products of H-burning at high temperatures (the main final product being
He).A. Bragaglia, Alonso, Alves, Anderson, Bastian, Bedin, Carretta, Carretta, Carretta, Carretta, Carretta, Carretta, Carretta, Carretta, Carretta, Carretta, Carretta, Cassisi, Castellani, Castellani, Catelan, Cohen, D'Antona, D'Antona, D'Antona, D'Antona, Decressin, E. Carretta, Ferraro, Glatt, Gratton, Gratton, Gratton, Harris, Iben., Kaviraj, Lee, Lee, Mackey, Marino, Marín-Franch, Milone, Milone, Milone, Moehler, Moretti, Norris, Pietrinferni, Pietrinferni, Pietrinferni, Piotto, Piotto, R. Gratton, S. Cassisi, S. Lucatello, Salaris, Salaris, Skrutskie, V. D'Orazi, Ventura, Ventura, Villanova, von Braun, Yong, Zoccali +64 morecore +1 more sourceA differential chemical abundance scale for the globular cluster M5
, 2010 We present LTE chemical abundances for five red giants and one AGB star in
the Galactic globular cluster (GC) M5 based on high resolution spectroscopy
using the MIKE spectrograph on the Magellan 6.5-m Clay telescope.Andreas Koch, Andrew McWilliam, Buonanno, Cassisi, Catelan, Cohen, Cutri, De Angeli, Dinescu, Ferguson, Fulbright, Fulbright, Fulbright, Fulbright, Fulbright, Gratton, Hanson, Ivans, Iwamoto, Koch, Koch, Koch, Layden, Nissen, Pietrinferni, Prochaska, Ramírez, Sandquist, Schlegel, Skrutskie, Stephens, Stetson, VandenBerg, Winkler, Yong, Yong +35 morecore +1 more source
