Results 1 to 10 of about 741,496 (215)
NGC1818 unveils the origin of the extended main-sequence turn-off in young Magellanic Clouds clusters [PDF]
Nature Communications, 2022 The nature of young star clusters in the Magellanic Clouds is debated. Here, the authors show an alternative approach that exploits data to exclude the presence of age differences greater than a few million years among cluster stars in a very young ...Giacomo Cordoni, Antonino P. Milone, Anna F. Marino, Michele Cignoni, Edoardo P. Lagioia, Marco Tailo, Marília Carlos, Emanuele Dondoglio, Sohee Jang, Anjana Mohandasan, Maria V. Legnardi +10 moredoaj +2 more sourcesOGLE-ing the Magellanic System: Optical Reddening Maps of the Large and Small Magellanic Clouds from Red Clump Stars [PDF]
Astrophysical Journal Supplement Series, 2020 We present the most extensive and detailed reddening maps of the Magellanic Clouds (MCs) derived from the color properties of Red Clump (RC) stars. The analysis is based on the deep photometric maps from the fourth phase of the Optical Gravitational ...D. Skowron, J. Skowron, A. Udalski, M. Szymański, I. Soszyński, Ł. Wyrzykowski, K. Ulaczyk, R. Poleski, S. Kozłowski, P. Pietrukowicz, P. Mróz, K. Rybicki, P. Iwanek, M. Wrona, M. Gromadzki +14 moresemanticscholar +1 more sourceEmpirical Calibration of the Reddening Maps in the Magellanic Clouds [PDF]
Astrophysical Journal, 2020 We present reddening maps of the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC), based on color measurements of the red clump. Reddening values of our maps were obtained by calculating the difference of the observed and intrinsic color of ...M. Górski, B. Zgirski, G. Pietrzyński, W. Gieren, P. Wielgórski, D. Graczyk, R. Kudritzki, B. Pilecki, W. Narloch, P. Karczmarek, K. Suchomska, M. Taormina +11 moresemanticscholar +1 more sourceGaia Early Data Release 3: Structure and properties of the Magellanic Clouds [PDF]
, 2020 We compare the Gaia DR2 and Gaia EDR3 performances in the study of the Magellanic Clouds and show the clear improvements in precision and accuracy in the new release.Gaia Collaboration, A. Brown, A. Vallenari, T. Prusti, J. Bruijne, C. Babusiaux, M. Biermann, O. Creevey, D. Evans, L. Eyer, A. Hutton, F. Jansen, C. Jordi, S. Klioner, U. Lammers, L. Lindegren, X. Luri, F. Mignard, C. Panem, D. Pourbaix, S. Randich, P. Sartoretti, C. Soubiran, N. Walton, Frédéric Arenou, C. Bailer-Jones, U. Bastian, M. Cropper, R. Drimmel, D. Katz, M. Lattanzi, F. V. Leeuwen, J. Bakker, C. Cacciari, J. Castañeda, F. Angeli, C. Ducourant, C. Fabricius, M. Fouesneau, Y. Fr'emat, R. Guerra, A. Guerrier, J. Guiraud, A. Piccolo, E. Masana, R. Messineo, N. Mowlavi, C. Nicolas, K. Nienartowicz, F. Pailler, P. Panuzzo, F. Riclet, W. Roux, G. Seabroke, R. Sordo, P. Tanga, F. Th'evenin, G. Gracia-Abril, J. Portell, D. Teyssier, M. Altmann, R. Andrae, I. Bellas-Velidis, K. Benson, J. Berthier, R. Blomme, E. Brugaletta, P. Burgess, G. Busso, B. Carry, A. Cellino, N. Cheek, G. Clementini, Y. Damerdji, M. Davidson, L. Delchambre, A. Dell’Oro, J. Fern'andez-Hern'andez, L. Galluccio, P. Garc'ia-Lario, M. Garcia-Reinaldos, J. Gonz'alez-N'unez, E. Gosset, R. Haigron, J. Halbwachs, N. Hambly, D. Harrison, D. Hatzidimitriou, U. Heiter, J. Hern'andez, D. Hestroffer, S. Hodgkin, B. Holl, K. Janssen, G. D. Fombelle, S. Jordan, A. Krone-Martins, A. Lanzafame, W. L. offler, A. Lorca, M. Manteiga, O. Marchal, P. Marrese, A. Moitinho, A. Mora, K. Muinonen, P. Osborne, E. Pancino, T. Pauwels, J. Petit, A. Recio-Blanco, P. J. Richards, M. Riello, L. Rimoldini, A. Robin, T. Roegiers, J. Rybizki, L. Sarro, C. Siopis, M. Smith, A. Sozzetti, A. Ulla, E. Utrilla, M. V. Leeuwen, W. V. Reeven, U. Abbas, A. Aramburu, S. Accart, C. Aerts, J. J. Aguado, M. Ajaj, G. Altavilla, M. A. Álvarez, J. '. Cid-Fuentes, J. Alves, R. I. Anderson, E. A. Varela, T. Antoja, M. Audard, D. Baines, S. Baker, L. Balaguer-N'unez, E. Balbinot, Z. Balog, C. Barache, D. Barbato, M. Barros, M. Barstow, S. Bartolom'e, J.-L. Bassilana, N. Bauchet, A. Baudesson-Stella, U. Becciani, M. Bellazzini, M. Bernet, S. Bertone, L. Bianchi, Sergi Blanco-Cuaresma, T. Boch, A. Bombrun, D. Bossini, S. Bouquillon, A. Bragaglia, L. Bramante, E. Breedt, A. Bressan, N. Brouillet, B. Bucciarelli, A. Burlacu, D. Busonero, A. Butkevich, R. Buzzi, E. Caffau, R. Cancelliere, H. C'anovas, T. Cantat-Gaudin, R. Carballo, T. Carlucci, M. I. Carnerero, J. Carrasco, L. Casamiquela, M. Castellani, A. Castro-Ginard, P. Sampol, L. Chaoul, P. Charlot, L. Chemin, A. Chiavassa, M. Cioni, G. Comoretto, W. J. Cooper, T. Cornez, S. Cowell, F. Crifo, M. Crosta, C. Crowley, C. Dafonte, A. Dapergolas, M. David, P. David, P. Laverny, F. Luise, R. March, J. Ridder, R. D. Souza, P. D. Teodoro, A. Torres, E. F. D. Peloso, E. D. Pozo, M. Delbo’, A. Delgado, H. E. Delgado, J. Delisle, P. Matteo, S. Diakite, C. Diener, E. Distefano, C. Dolding, D. Eappachen, B. Edvardsson, H. Enke, P. Esquej, C. Fabre, M. Fabrizio, S. Faigler, G. Fedorets, P. Fernique, A. Fienga, F. Figueras, C. Fouron, F. Fragkoudi, E. Fraile, F. Franke, M. Gai, D. Garabato, A. García-Gutiérrez, M. Garc'ia-Torres, A. Garofalo, P. Gavras, E. Gerlach, R. Geyer, P. Giacobbe, G. Gilmore, S. Girona, G. Giuffrida, R. Gomel, A. Gómez, I. González-Santamaría, J. J. Gonz'alez-Vidal, M. Granvik, R. Guti'errez-S'anchez, L. Guy, M. Hauser, M. Haywood, A. Helmi, S. Hidalgo, T. Hilger, N. Hładczuk, D. Hobbs, G. Holland, H. Huckle, G. Jasniewicz, P. Jonker, J. Campillo, F. Julbé, L. Karbevska, P. Kervella, S. Khanna, A. Kochoska, M. Kontizas, G. Kordopatis, A. Korn, Z. Kostrzewa-Rutkowska, K. Kruszy'nska, S. Lambert, A. Lanza, Y. Lasne, J. L. Campion, Y. L. Fustec, Y. Lebreton, T. Lebzelter, S. Leccia, N. Leclerc, I. Lecoeur-Taibi, S. Liao, E. Licata, H. Lindstrøm, T. Lister, E. Livanou, A. Lobel, P. Pardo, S. Managau, R. Mann, J. Marchant, M. Marconi, M.M.S. Marcos Santos, S. Marinoni, F. Marocco, D. Marshall, L. M. Polo, J. Mart'in-Fleitas, A. Masip, D. Massari, A. Mastrobuono-Battisti, T. Mazeh, P. McMillan, S. Messina, D. Michalik, N. Millar, A. Mints, D. Molina, R. Molinaro, L. Moln'ar, P. Montegriffo, R. Mor, R. Morbidelli, T. Morel, D. Morris, A. Mulone, D. Munoz, T. Muraveva, C. P. Murphy, I. Musella, L. Noval, C. Ord'enovic, G. Orrú, J. Osinde, C. Pagani, I. Pagano, L. Palaversa, P. Palicio, A. Panahi, M. Pawlak, X. P. Esteller, A. a, A. Piersimoni, F. Pineau, E. Plachy, G. Plum, E. Poggio, E. Poretti, E. Poujoulet, A. Prvsa, L. Pulone, E. Racero, S. Ragaini, M. Rainer, C. Raiteri, N. Rambaux, P. Ramos, M. Ramos-Lerate, P. Fiorentin, S. Regibo, C. Reyl'e, V. Ripepi, A. Riva, G. Rixon, N. Robichon, C. Robin, M. Roelens, L. Rohrbasser, M. Romero-G'omez, N. Rowell, F. Royer, K. Rybicki, G. Sadowski, A. S. Sell'es, J. Sahlmann, J. Salgado, E. Salguero, N. Samaras, V. S. Gimenez, N. Sanna, R. Santoveña, M. Sarasso, M. Schultheis, E. Sciacca, M. Ségol, J. Segovia, D. S'egransan, D. Semeux, S. Shahaf, H. Siddiqui, A. Siebert, L. Siltala, É. Slezak, R. Smart, E. Solano, F. Solitro, D. Souami, J. Souchay, A. Spagna, F. Spoto, I. Steele, H. S. uller, C. Stephenson, M. uveges, L. Szabados, E. Szegedi-Elek, F. Taris, G. Tauran, M. B. Taylor, R. Teixeira, W. Thuillot, N. Tonello, F. Torra, J. Torra, C. Turon, N. Unger, M. Vaillant, E. W. Dillen, O. Vanel, A. Vecchiato, Y. Viala, D. Vicente, S. Voutsinas, M. Weiler, T. Wevers, L. Wyrzykowski, A. Yoldas, P. Yvard, H. Zhao, J. Zorec, S. Zucker, C. Zurbach, T. Zwitter +425 moresemanticscholar +1 more sourceDiscovery of the Magellanic Stellar Stream Out to 100 kpc
The Astrophysical Journal, 2023 The Magellanic Stream (MS)—an enormous ribbon of gas spanning 140° of the southern sky trailing the Magellanic Clouds—has been exquisitely mapped in the five decades since its discovery.Vedant Chandra, Rohan P. Naidu, Charlie Conroy, Ana Bonaca, Dennis Zaritsky, Phillip A. Cargile, Nelson Caldwell, Benjamin D. Johnson, Jiwon Jesse Han, Yuan-Sen Ting +9 moredoaj +1 more sourceMagellanic Clouds Cepheids: Thorium Abundances [PDF]
Journal of Astronomy and Space Sciences, 2018 The analysis of the high-resolution spectra of 31 Magellanic Clouds Cepheid variables enabled the identification of thorium lines. The abundances of thorium were found with spectrum synthesis method. The calculated thorium abundances exhibit correlations Yeuncheol Jeong, Alexander V. Yushchenko, Vira F. Gopka, Volodymyr O. Yushchenko, Valery V. Kovtyukh, Svetlana V. Vasil’eva +5 moredoaj +1 more sourceThe Missing Satellites of the Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-faint Galaxies [PDF]
Astrophysical Journal, 2018 According to LCDM theory, hierarchical evolution occurs on all mass scales, implying that satellites of the Milky Way should also have companions. The recent discovery of ultra-faint dwarf galaxy candidates in close proximity to the Magellanic Clouds ...N. Kallivayalil, L. Sales, P. Zivick, T. Fritz, Andrés del Pino, S. Sohn, G. Besla, R. P. van der Marel, J. Navarro, E. Sacchi +9 moresemanticscholar +1 more source