Results 61 to 70 of about 108,892 (343)
The AIMSS Project, III : the stellar populations of compact stellar systems [PDF]
, 2015 In recent years, a growing zoo of compact stellar systems (CSSs) have been found whose physical properties (mass, size, velocity dispersion) place them between classical globular clusters (GCs) and true galaxies, leading to debates about their nature ...Brodie, Jean, Escudero, Carlos Gabriel, Faifer, Favio Raúl, Forbes, Duncan A., Forte, Juan Carlos, Frank, Matthias, Huxor, Avon, Janz, Joachin, Kannappan, Sheila J., Maraston, Claudia, Norris, Mark A., Romanowsky, Aaron, Strader, Jay, Thompson, Bradley +13 morecore +6 more sourcesSTELLAR POPULATION VARIATIONS IN THE MILKY WAY's STELLAR HALO [PDF]
The Astronomical Journal, 2010 If the stellar halos of disk galaxies are built up from the disruption of dwarf galaxies, models predict highly structured variations in the stellar populations within these halos. We test this prediction by studying the ratio of blue horizontal branch stars (BHB stars; more abundant in old, metal-poor populations) to main-sequence turn-off stars (MSTO Bell, Eric F., Xue, Xiang Xiang, Rix, Hans-Walter, Ruhland, Christine, Hogg, David W. +4 moreopenaire +2 more sourcesStereotactic Body Radiation Therapy for Pediatric, Adolescent, and Young Adult Patients With Osteosarcoma: Local Control Outcomes With Dosimetric Analysis
Pediatric Blood &Cancer, EarlyView.ABSTRACT Background/Objectives
Osteosarcoma is a radioresistant tumor that may benefit from stereotactic body radiation therapy (SBRT) for locoregional control in metastatic/recurrent disease. We report institutional practice patterns, outcomes, toxicity, and failures in osteosarcoma patients treated with SBRT.Jenna Kocsis, Shauna R. Campbell, Jonathan Jang, Eashwar Somasundaram, Chandana A. Reddy, Jacob G. Scott, Lilyana Angelov, Peter M. Anderson, Matteo Trucco, Zachary Burke, Lukas Nystrom, Nathan Mesko, Anthony Magnelli, Erin S. Murphy +13 morewiley +1 more sourceIntracluster Stellar Population [PDF]
Symposium - International Astronomical Union, 2004 I shall review the latest results for the presence of diffuse light in nearby clusters, and the evidence of ongoing star formation in an intracluster Virgo field. I shall discuss how intracluster planetary nebulae (ICPN) can be used as excellent tracers of the diffuse stellar population in nearby clusters.openaire +2 more sourcesStellar population trends in S0 galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2010 We present stellar population age and metallicity trends for a sample of 59 S0 galaxies based on optical Sloan Digital Sky Survey (SDSS) and near-infrared (NIR)Mcdonald, Michael, Chamberlain, L. C.Prochaska, Courteau, Stéphane, Rose, James A. +3 moreopenaire +1 more sourceThe stellar and sub-stellar IMF of simple and composite populations
, 2012 The current knowledge on the stellar IMF is documented. It appears to become
top-heavy when the star-formation rate density surpasses about 0.1Msun/(yr
pc^3) on a pc scale and it may become increasingly bottom-heavy with increasing
metallicity and in ...A Duquennoy, A Maeder, A Parravano, A Sollima, A Sollima, A Stolte, A Vazdekis, A Vazdekis, AA Muench, AE Piskunov, AJ Cenarro, AN Belikov, AP Whitworth, AR Boss, AS Eddington, AT Myers, B Binggeli, B García, B Reipurth, BG Elmegreen, BG Elmegreen, BG Elmegreen, BG Elmegreen, BG Elmegreen, BG Elmegreen, BG Elmegreen, BG Elmegreen, BG Elmegreen, C Briceño, C Esteban, C Flynn, C Grillo, C Hayashi, C Koen, C Low, C Reylé, C Soubiran, C Weidner, C Weidner, C Weidner, C Weidner, C Weidner, C Weidner, C Weidner, C Yasui, CA Tout, CJ Clarke, CJ Grillmair, CJ Lada, CJ Lonsdale, CL Slesnick, CM Baugh, CM Boily, D Calzetti, D Gouliermis, D Gouliermis, D Stamatellos, D Stamatellos, D Stamatellos, D Stamatellos, D Vanbeveren, DA Fischer, DA Forbes, DA Tilley, DA Tilley, DC Heggie, DF Figer, DJ Pinfield, DJ Price, DR Weisz, E Brocato, E Casuso, E Corbelli, E Moraux, E Schilbach, E Vesperini, E Vesperini, EA Evstigneeva, EA Hoversten, EE Salpeter, F D’Antona, F Egusa, F Motte, F Najarro, F Palla, F Paresce, F Selman, FC Adams, FC Adams, FD Kahn, G Basri, G Bosch, G Chabrier, G Chabrier, G Chabrier, G Chabrier, G Chabrier, G Chabrier, G Duchêne, G Garcia-Segura, G Garcia-Segura, G Marchi de, G Marchi de, G Marchi De, G Piotto, G Weigelt, G Wuchterl, G Wuchterl, GE Miller, GR Blumenthal, GR Meurer, H Bartko, H Baumgardt, H Baumgardt, H Bouy, H Jahreiss, H Kirk, H Sana, H Zinnecker, H Zinnecker, HT Janka, I Baraffe, I Misgeld, I Thies, I Thies, I Thies, I Thies, IA Bonnell, IA Bonnell, IA Bonnell, IA Bonnell, IA Bonnell, IA Bonnell, IN Reid, IN Reid, IN Reid, IN Reid, J Binney, J Bouvier, J Dabringhausen, J Dabringhausen, J Dabringhausen, J Jijina, J Köppen, J Maíz Apellániz, J Maíz Apellániz, J Maíz Apellániz, J Pflamm-Altenburg, J Pflamm-Altenburg, J Pflamm-Altenburg, J Pflamm-Altenburg, J Pflamm-Altenburg, J Pflamm-Altenburg, J Pflamm-Altenburg, J Pflamm-Altenburg, J Strader, JB Lamb, JC Tan, JD Neill, JE Dale, JE Gizis, JH Jeans, JJ Bochanski, JL Beuzit, JL Halbwachs, JM Kirk, JM Oliveira, JM Scalo, JN Bahcall, JP Anderson, JS Kalirai, JS Ulvestad, K Fuhrmann, K Kuijken, KD Finkelstein, KL Luhman, KL Luhman, KS Boer de, L Siess, L Testi, LA Hillenbrand, LA Hillenbrand, LJ Smith, LM Close, LR Penny, M Andersen, M Andersen, M Beech, M Dominik, M Fellhauer, M Fellhauer, M Fellhauer, M Fellhauer, M Fumagalli, M Haywood, M Mac Low, M Marks, M Marks, M Marks, M Marks, M Marks, M Marks, M Nagashima, M Ramspeck, M Schmalzl, M Schwarzschild, M Sirianni, MA Pérez-Torres, MG Wolfire, MJ Disney, MN Machida, MN Machida, MR Bate, MR Bate, MR Bate, MR Krumholz, MR Krumholz, MR Krumholz, MS Oey, MS Oey, N Bastian, N Ivanova, N Kevlahan, N Lodieu, N McCrady, N Moeckel, N Murray, N Phan-Bao, N Reid, N Rio Da, NC Hambly, NC Hambly, O Malkov, OY Malkov, P Girichidis, P Hennebelle, P Hennebelle, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Kroupa, P Massey, P Massey, P Padoan, P Padoan, P Wang, PA Crowther, PC Clark, PC Myers, PFL Maxted, PG Dokkum van, PG Dokkum van, PJE Peebles, PP Papadopoulos, PP Papadopoulos, PR Allen, R Chini, R Fuente Marcos de La, R Kudritzki, R Parra, R Wojtak, R Wünsch, RB Larson, RB Larson, RB Stothers, RC Kennicutt Jr, RJ Parker, RJ Parker, RJ Parker, RJ Smith, RJ White, RS Klessen, RS Klessen, RS Stobie, S Banerjee, S Basu, S Basu, S Bontemps, S Dib, S Dib, S Djorgovski, S Feltzing, S Hocuk, S Mieske, S Mieske, S Nayakshin, S Recchi, S Roychowdhury, S Röser, S Shen, S Zucker, SD Murray, SF Portegies Zwart, SJ Aarseth, SLW McMillan, SM Wilkins, SP Goodwin, SP Goodwin, SP Goodwin, SP Goodwin, SP Goodwin, SS Kim, SS Vogt, ST Megeath, T Chlebowski, T Hippel von, T Maschberger, T Maschberger, T Maschberger, T Onishi, T Peters, T Peters, T Preibisch, T Tsujimoto, TE Lutz, TJ Henry, TV Veltchev, U Löckmann, V Bromm, V Joergens, V Weidemann, VV Gvaramadze, VV Gvaramadze, W Jao, W-H Hsu, WJ Wit de, WJ Wit de, X Delfosse, X Delfosse, Y Li, Z-Y Li, Å Nordlund +344 morecore +1 more sourceMULTIPLE STELLAR POPULATIONS IN 47 Tucanae [PDF]
The Astrophysical Journal, 2011 49 pages, 35 figures, accepted for pubblication in ...MILONE, ANTONINO, PIOTTO, GIAMPAOLO, BEDIN, LUIGI, KING, IVAN ROBERT, J. Anderson, MARINO, ANNA, BELLINI, ANDREA, R. Gratton, A. Renzini, STETSON, PETER B., S. Cassisi, A. Aparicio, A. Bragaglia, E. Carretta, F. D'Antona, M. . Criscienzo, S. Lucatello, M. Monelli, A. Pietrinferni +18 moreopenaire +4 more sources
