Results 21 to 30 of about 228,068 (290)
UGC 7388: a galaxy with two tidal loops
, 2009 We present the results of spectroscopic and morphological studies of the
galaxy UGC7388 with the 8.1-m Gemini North telescope. Judging by its observed
characteristics, UGC7388 is a giant late-type spiral galaxy seen almost
edge-on.B. C. Whitmore, Ch. Brocca, F. Schweizer, G. Monnet, I. F. Fernandes, J. Dubinski, J. K. Adelman-McCarthy, K. O’Neil, L. Bottinelli, M. de Oliveira-Abans, M. Faúndez-Abans, M. R. Blanton, O. K. Silchenko, R. A. Ibata, R. B. Tully, R. B. Tully, R. Ibata, V. P. Reshetnikov, V. P. Reshetnikov, V. P. Reshetnikov, V. Reshetnikov, V. Reshetnikov, V. Reshetnikov, Zh. Shang +23 morecore +1 more sourceA galaxy-halo model of large-scale structure [PDF]
, 2005 We present a new, galaxy-halo model of large-scale structure, in which the
galaxies entering a given sample are the fundamental objects. Haloes attach to
galaxies, in contrast to the standard halo model, in which galaxies attach to
haloes.Andrew J. S. Hamilton, Berlind, Coles, Cooray, Dekel, Guzik, Hamilton, Hamilton, Hoekstra, Ma, Mandelbaum, Mark C. Neyrinck, Navarro, Neyman, Neyrinck, Neyrinck, Nickolay Y. Gnedin, Peacock, Peebles, Pen, Scherrer, Scoccimarro, Seljak, Seljak, Seljak, Seljak, Sheldon, Sheth, Taruya, Tasitsiomi, Tegmark, Zehavi +31 morecore +3 more sourcesUnravelling the origin of large-scale magnetic fields in galaxy clusters
and beyond through Faraday Rotation Measures with the SKA [PDF]
, 2014 We investigate the possibility for the SKA to detect and study the magnetic
fields in galaxy clusters and in the less dense environments surrounding them
using Faraday Rotation Measures.Akahori, T., Bonafede, A., Brüggen, M., Carretti, E., Colafrancesco, S., Feretti, L., Ferrari, C., Giovannini, G., Govoni, F., Govoni, F., Johnston-Hollitt, M., Murgia, M., Rudnick, L., Scaife, A., Scaife, A., Vacca, V., Vazza, F. +16 morecore +2 more sourcesMRC B0319-454: Probing the large-scale structure with a giant radio
galaxy
, 2008 We present an investigation of the relationships between the radio properties
of a giant radio galaxy MRC B0319-454 and the surrounding galaxy distribution
with the aim of examining the influence of intergalactic gas and gravity
associated with the large-Begelman, Bliton, Blundell, Boehringer, Bregman, Bryant, Brüggen, Bîrzan, Cen, Cen, Churazov, Davé, Douglass, Fleenor, Fleenor, G. V. Bicknell, Gull, Hardcastle, Hardcastle, Haslam, Haverkorn, Huchra, Ishwara-Chandra, Jamrozy, Jamrozy, Jones, Jones, Jones, Kaiser, Kaiser, Klamer, Kraft, L. Saripalli, Lara, Ledlow, Lewis, McNamara, Mills, Mulchaey, Nulsen, R. Subrahmanyan, Safouris, Saripalli, Schatzmann, Scheuer, Simard-Normandin, Slee, Subrahmanyan, V. Safouris, Worrall, Worrall, Wright +51 morecore +1 more sourceGalaxy Formation Theory [PDF]
, 2010 We review the current theory of how galaxies form within the cosmological
framework provided by the cold dark matter paradigm for structure formation.
Beginning with the pre-galactic evolution of baryonic material we describe the
analytical and numerical Abadi, Abadi, Abel, Abel, Abel, Abraham, Agertz, Ahn, Allen, Andrew J. Benson, Angus, Arad, Arons, Athanassoula, Athanassoula, Aubert, Bahcall, Bahcall, Banerjee, Bardeen, Barnes, Barnes, Barnes, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Begelman, Begelman, Bell, Belokurov, Belokurov, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Berezinsky, Berti, Bertin, Bertone, Bertschinger, Bertschinger, Bett, Binney, Binney, Birnboim, Birzan, Blaizot, Blaizot, Blaizot, Blanchet, Bland-Hawthorn, Blandford, Blandford, Blumenthal, Blumenthal, Bode, Boehm, Bond, Bondi, Booth, Borgani, Bournaud, Bournaud, Bower, Bower, Bower, Bower, Boylan-Kolchin, Boyle, Bromm, Bromm, Brook, Brook, Brooks, Bruzual, Brüggen, Brüggen, Bullock, Bullock, Bullock, Bullock, Cardone, Cattaneo, Cazaux, Chabrier, Chakrabarti, Chandrasekhar, Chary, Chiu, Christodoulou, Christodoulou, Ciardi, Ciardi, Ciotti, Clarke, Clarke, Cole, Cole, Cole, Cole, Cole, Cole, Cole, Colín, Conroy, Conroy, Conroy, Cooray, Covington, Cox, Cox, Crain, Croton, Croton, Davis, Davé, de Vaucouleurs, Dekel, Devriendt, Devriendt, Diaferio, Dolag, Dotter, Dove, Draine, Dunkley, Dutton, Dutton, Edgar, Efstathiou, Efstathiou, Efstathiou, Einasto, Eisenstein, Eke, Eke, El-Zant, Elahi, Fakhouri, Fakhouri, Fall, Fan, Fardal, Favata, Federrath, Ferland, Ferrara, Ferrarese, Ferrarese, Field, Finlator, Firmani, Fitchett, Font, Font, Font, Font, Fontanot, Fontanot, François, Freeman, Frenk, Frenk, Frenk, Friedli, Fryxell, Galli, Gao, Gao, Gebhardt, Gebhardt, Glover, Gnat, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Goerdt, Goldreich, Gonçalves, Gould, Governato, Governato, Governato, Granato, Greif, Guiderdoni, Gunn, Gunn, Guo, Gustafsson, Haardt, Hahn, Hamilton, Harris, Hatton, Heitmann, Helly, Helly, Henriques, Hernquist, Hollenbach, Hoyle, Hubble, Jenkins, Jenkins, Jiang, Jing, Jog, Johnston, Jonsson, Jubelgas, Kampakoglou, Kant, Katz, Katz, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kaufmann, Kay, Kazantzidis, Kennicutt, Kennicutt, Kereš, Kereš, King, King, King, Klypin, Klypin, Klypin, Kobayashi, Komatsu, Komissarov, Kormendy, Kormendy, Kormendy, Kowalski, Kravtsov, Kravtsov, Kravtsov, Kriek, Kroupa, Krumholz, Kuhlen, Kuijken, Lacey, Lacey, Lacey, Lacey, Lanzoni, Larson, Laursen, Law, Lawlor, Lee, Lemson, Li, Li, Libeskind, Lin, Lin, Lintott, Lotz, Lotz, Lucia, Lucia, Lucia, Lynden-Bell, Lynden-Bell, Machida, Madau, Madau, Madau, Magorrian, Malbon, Maller, Maller, Maller, Maller, Mandelbaum, Mao, Maraston, Marigo, Marri, Martin, Martínez-Serrano, Mastropietro, Mastropietro, Mateo, Matteo, Matteo, Matteo, Matteucci, Matteucci, Mayer, Mayer, McCarthy, McCarthy, McDowell, McKee, McKee, Meier, Meier, Meiksin, Merritt, Merritt, Milosavljevic, Milosavljevic, Minchev, Miranda, Mo, Monaco, Monaco, Monaco, Moore, Moore, Moore, Moore, Moore, Murali, Murali, Murali, Murray, Nagashima, Nagashima, Narayan, Narayanan, Narlikar, Navarro, Navarro, Navarro, Navarro, Navarro, Navarro, Neistein, Nemmen, Neyman, Nulsen, Ocvirk, Okamoto, Okamoto, Omma, Oppenheimer, Ostriker, Owen, O’Shea, O’Shea, Padilla, Parkinson, Parrish, Parry, Peacock, Peacock, Peebles, Percival, Percival, Peters, Petkova, Pipino, Pipino, Plewa, Pontzen, Pope, Portinari, Prada, Press, Purcell, Putman, Quilis, Quinlan, Quinlan, Quinn, Randall, Rasmussen, Ratnatunga, Razoumov, Read, Read, Reed, Reed, Rees, Ricker, Ricotti, Ricotti, Ricotti, Rijkhorst, Robertson, Robertson, Robertson, Robertson, Robertson, Robinson, Romano, Romeo, Romeo, Roskar, Roskar, Roychowdhury, Rozo, Ruszkowski, Ruszkowski, Sales, Salpeter, Santoro, Scannapieco, Scannapieco, Scannapieco, Scannapieco, Schade, Schawinski, Schaye, Schmidt, Seljak, Sellwood, Sellwood, Sellwood, Sesana, Sesana, Shakura, Shapiro, Sharma, Shaw, Shen, Sheth, Shlosman, Sijacki, Silk, Silk, Silk, Silva, Simard, Slosar, Smith, Smith, Smoluchowksi, Somerville, Somerville, Somerville, Somerville, Somerville, Somerville, Spitzer, Spitzer, Springel, Springel, Springel, Springel, Springel, Springel, Stacy, Steinmetz, Stewart, Stinson, Strigari, Summers, Swinbank, Tasker, Tasker, Tassis, Taylor, Tegmark, Tegmark, Tegmark, Thacker, Thacker, Thorne, Tichy, Timmes, Tinker, Tinker, Tollerud, Toomre, Tormen, Toth, Tozzi, Tremaine, Tremaine, Trenti, Tumlinson, van den Bosch, van den Bosch, van den Bosch, van Dokkum, Vecchia, Vecchia, Veilleux, Velazquez, Vernaleo, Viel, Vikhlinin, Villalobos, Villiers, Vitvitska, Voit, Volonteri, Volonteri, Volonteri, Wadsley, Wang, Wang, Wang, Warren, Watanabe, Wechsler, Wechsler, Wen, White, White, White, White, White, Williams, Willman, Wise, Wise, Wise, Wise, Wise, Wise, Wuyts, Wyithe, Yajima, Yang, Yoshida, Yoshida, Yoshida, Younger, Younger, Yu, Yüksel, Zavala, Zhang, Zhao, Zhao, Zheng +563 morecore +1 more sourceChaotic Spiral Galaxies
, 2011 We study the role of asymptotic curves in supporting the spiral structure of
a N-body model simulating a barred spiral galaxy. Chaotic orbits with initial
conditions on the unstable asymptotic curves of the main unstable periodic
orbits follow the shape ...Contopoulos, George, Harsoula, Mirellacore +1 more source
