Results 41 to 50 of about 36,167 (318)
Hot stars in globular clusters [PDF]
, 1995 Globular clusters are ideal laboratories to study the evolution of low-mass stars. In this review, I shall concentrate on two types of hot stars observed in globular clusters: horizontal branch stars and UV bright stars. The third type, the white dwarfs, are covered by Bono in this volume.Ulrich Heber, Klaas S. de Boer, Sabine Moehler +2 moreopenaire +2 more sourcesChemical evolution of star clusters
, 2009 I discuss the chemical evolution of star clusters, with emphasis on old
globular clusters, in relation to their formation histories. Globular clusters
clearly formed in a complex fashion, under markedly different conditions from
any younger clusters ...Abia C., Charbonnel C., Dubath P., Mackey A. D., Romano D., van Loon J. Th., Yi S. K. +6 morecore +1 more sourceThe Colors of Dwarf Elliptical Galaxy Globular Cluster Systems, Nuclei
and Stellar Halos
, 2004 We present the results of a Hubble Space Telescope WFPC2 F555W and F814W
survey of 69 dwarf elliptical galaxies (dEs) in the Virgo and Fornax Clusters
and Leo Group.Arimoto N., Babul A., Binggeli B., Bryan W. Miller, Drinkwater M. J., Fall S. M., Grebel E., Henry C. Ferguson, Jennifer M. Lotz, Kauffmann G., Thomas D. +10 morecore +1 more sourceMassive star cluster formation and evolution in tidal dwarf galaxies [PDF]
, 2019 Reproduced with permission from Astronomy & Astrophysics. © 2019 ESOThe formation of globular clusters remains an open debate. Dwarf starburst galaxies are efficient at forming young massive clusters with similar masses as globular clusters and may hold ...Boquien, Mederic, Bournaud, Frederic, Brinks, Elias, Duc, Pierre-Alain, Elmegreen, Bruce G., Elmegreen, Debra M., Fensch, Jeremy, Grijs, Richard de, Lelli, Federico, Renaud, Florent, Weilbacher, Peter M. +10 morecore +4 more sourcesThe ESO-VLT MIKiS Survey Reloaded: Exploring the Internal Kinematics of NGC 6440
The Astrophysical Journal, 2023 In the context of the ESO-VLT Multi-Instrument Kinematic Survey of Galactic globular clusters, here we present the line-of-sight velocity dispersion profile of NGC 6440, a massive globular cluster located in the Galactic bulge.Silvia Leanza, Cristina Pallanca, Francesco R. Ferraro, Barbara Lanzoni, Emanuele Dalessandro, Mario Cadelano, Enrico Vesperini, Livia Origlia, Alessio Mucciarelli, Elena Valenti +9 moredoaj +1 more sourceTHE SEQUENTIAL STAR FORMATION IN GLOBULAR CLUSTERS
Odessa Astronomical Publications, 2008 The results of [O/Na] abundance modelling in globular clusters NGC 2808 and NGC 6752 are presented. The evolutionary scenario allowing to reproduce characteristic observed features of [O/Na] distribution function has been suggested.M. V. Ryabova, Yu. A. Shchekinovdoaj +1 more sourceMultiple 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 source
