Results 91 to 100 of about 12,590,287 (391)
The Stability of Some Galaxy Disks is Still Perplexing
The Astrophysical Journal, 2023 The problem of how some disk galaxies avoid forming bars remains unsolved. Many galaxy models having reasonable properties continue to manifest vigorous instabilities that rapidly form strong bars and no widely accepted idea has yet been advanced to ...J. A. Sellwood, R. G. Carlbergdoaj +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 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 sourceCrawling the Cosmic Network: Exploring the Morphology of Structure in
the Galaxy Distribution [PDF]
, 2010 Although coherent large-scale structures such as filaments and walls are
apparent to the eye in galaxy redshift surveys, they have so far proven
difficult to characterize with computer algorithms. This paper presents a
procedure that uses the eigenvalues Abazajian, Aragón-Calvo, Barrow, Berlind, Blanton, Bond, Bond, Colberg, Colless, Colombi, Davis, De Lapparent, Dietrich, Eisenstein, Forero-Romero, Frenk, Fry, Gaztanaga, Geller, Gott, Guth, Hahn, Huchra, Klypin, Kulkarni, Lee, Martínez, Massey, Michael A. Strauss, Nichol, Nicholas A. Bond, Novikov, Pan, Park, Peebles, Press, Renyue Cen, Roberts, Ross, Schaap, Shandarin, Shen, Smith, Sousbie, Sousbie, Spergel, Stein, Strauss, Tanaka, Thompson, Verde, York, Zel'dovich, Zel'dovich, Zheng +54 morecore +1 more sourceRoll‐To‐Roll Production of Smart Dressings for Wound Monitoring
Advanced Healthcare Materials, EarlyView.This study presents a roll‐to‐roll manufactured smart wound dressing capable of visually monitoring key wound biomarkers, including pH, humidity, and temperature. By integrating colorimetric sensors into flexible dressing substrates, the device offers real‐time, equipment‐free insights for infection detection and wound management, representing a ...Ziheng Wang, Yujin Ahn, Semin Kwon, Tianhao Yu, Yumin Dai, Julia Walsh, Joo Hun Lee, Sang Mok Park, Seul Ah Lee, Murtuza Peerbhai, Chandan K. Sen, Hyowon Lee, Young L. Kim, Hyunjoon Kong, Chi Hwan Lee +14 morewiley +1 more source