Results 41 to 50 of about 36,679 (341)
Chemical 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 sourceAccretion of gas by globular cluster stars [PDF]
Astronomy & Astrophysics, 2002 11 pages; accepted for publication in Astronomy and ...Thoul, Anne, Jorissen, Alain, Goriely, Stéphane, Jehin, Emmanuel, Magain, Pierre, Noels, Arlette, Parmentier, Geneviève +6 moreopenaire +4 more sourcesJWST/NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc
The Astrophysical Journal, 2023 Star cluster formation in the early universe and its contribution to reionization
remains largely unconstrained to date. Here we present JWST/NIRCam imaging of
the most highly magnified galaxy known at z ∼ 6,
the Sunrise arc.Eros Vanzella, Adélaïde Claeyssens, Brian Welch, Angela Adamo, Dan Coe, Jose M. Diego, Guillaume Mahler, Gourav Khullar, Vasily Kokorev, Masamune Oguri, Swara Ravindranath, Lukas J. Furtak, Tiger Yu-Yang Hsiao, Abdurro’uf, Nir Mandelker, Gabriel Brammer, Larry D. Bradley, Maruša Bradač, Christopher J. Conselice, Pratika Dayal, Mario Nonino, Felipe Andrade-Santos, Rogier A. Windhorst, Nor Pirzkal, Keren Sharon, S. E. de Mink, Seiji Fujimoto, Adi Zitrin, Jan J. Eldridge, Colin Norman +29 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 sourceStar cluster formation and star formation: the role of environment and star-formation efficiencies [PDF]
, 2008 “The original publication is available at www.springerlink.com”. Copyright Springer. DOI: 10.1007/s10509-009-0088-5By analyzing global starburst properties in various kinds of starburst and post-starburst galaxies and relating them to the properties of ...A. Pasquali, A. Schulz, B.C. Whitmore, B.C. Whitmore, B.C. Whitmore, B.G. Elmegreen, B.W. Miller, C. Maraston, C.D. Wilson, C.D. Wilson, C.J. Jog, C.J. Jog, D. Calzetti, E. Hummel, F. Schweizer, F. Schweizer, F. Schweizer, F. Schweizer, G. Parmentier, G. Parmentier, G. Trancho, G. Worthey, G.R. Meurer, H. Krueger, J. Gorgas, J. Schulz, J.H. Brown, K.A. Knierman, M. Haas, M.D. Mora, O.M. Kurth, P. Anders, P. Anders, P. Anders, P. Anders, P. Goudfrooij, P. Goudfrooij, P. Goudfrooij, P. Goudfrooij, P.M. Solomon, R. Grijs de, R. Grijs de, S. Bergh van der, S.C. Gallagher, S.E. Zepf, S.G. Boutloukos, S.S. Larsen, S.S. Larsen, T. Lilly, T. Lilly, U. Fritze-v. Alvensleben, U. Fritze-v. Alvensleben, U. Fritze-v. Alvensleben, U. Fritze-v. Alvensleben, Uta Fritze, Y. Gao, Y. Gao, Y. Li, Y. Shioya +58 morecore +2 more sourcesHot 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 sourcesMultiple 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 sourceResolving Globular Cluster Formation within a Cosmological Context [PDF]
, 2009 We place constraints on the formation redshifts for blue globular clusters
(BGCs), independent of the details of hydrodynamics and population III star
formation.Aaron C. Boley, Ashman, Bastian, Baumgardt, Bertschinger, Binney, Binney, Bromm, de Angeli, Eisenstein, Fall, George Lake, Gnedin, Gnedin, Greif, Gunn, Harris, Hinshaw, Justin Read, Kravtsov, Levine, Madau, Moore, Nakamura, Romain Teyssier, Sarajedini, Schweizer, Surdin, Tumlinson, Woosley, Zhang +30 morecore +2 more sourcesStar-Forming Galaxies at z~2 and the Formation of the Metal-Rich
Globular Cluster Population
, 2010 We examine whether the super star-forming clumps (R~1-3 kpc; M~10^8-10^9.5
Msun) now known to be a key component of star-forming galaxies at z~2 could be
the formation sites of the locally observed old globular cluster population.Armandroff, Ashman, Barmby, Bournaud, Bournaud, Bridges, Brodie, Conroy, Cowie, Cresci, Côté, Côté, Daddi, De Angeli, de Grijs, Dekel, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elson, English, Erb, Erb, Escala, Fall, Forbes, Förster Schreiber, Förster Schreiber, Genel, Genzel, Genzel, Halliday, Harris, Huchra, Immeli, Jordán, Kristen L. Shapiro, Kuntschner, Mannucci, McLaughlin, McLaughlin, McLaughlin, Mendel, Minniti, Murray, Natascha M. Förster Schreiber, Noguchi, Peng, Peng, Peng, Pettini, Puzia, Quider, Reddy, Reinhard Genzel, Rhode, Rhode, Rudnick, Scannapieco, Schroder, Searle, Strader, Tacconi, Thomas, Trujillo, van den Bergh, Wilson, Zepf, Zinn +71 morecore +1 more source
