Results 51 to 60 of about 438,137 (232)
Calibration of radii and masses of open clusters with a simulation
, 2010 Context: A recent new approach to apply a simple dynamical mass estimate of
tidally limited star clusters is based on the identification of the tidal
radius in a King profile with the dynamical Jacobi radius.A. Ernst, A. Just, Aarseth, Casertano, Dauphole, Harfst, Just, Kharchenko, King, King, M. I. Petrov, Makino, Miller, Miyamoto, P. Berczik, Piskunov, Piskunov, Piskunov, Roeser, Spurzem, Wielen +20 morecore +1 more sourceRadio Triggered Star Formation in Cooling Flows
, 1999 The giant galaxies located at the centers of cluster cooling flows are
frequently sites of vigorous star formation. In some instances, star formation
appears to have been triggered by the galaxy's radio source.Allen, Allen, Allen, B.R. McNamara, Baum, Begelman, Burns, Cardiel, Crawford, Daly, De Young, di Serego Alighieri, Fabian, Heckman, Jannuzi, Johnstone, Koekemoer, McCarthy, McNamara, McNamara, McNamara, McNamara, McNamara, McNamara, Murphy, Pinkney, Porter, Sarazin, Sarazin, Schombert, Shields, Uson, van Breugel, van Breugel, Voit +34 morecore +2 more sourcesA Tale of Three Dwarfs: Cluster-based Star Formation Histories of Blue Compact Dwarf Galaxies
The Astrophysical JournalWe present a new study of the cluster populations in the blue compact dwarf galaxies (BCD) ESO185-IG13, ESO338-IG04, and Haro11, based on new and archival high-resolution images taken by the Hubble Space Telescope, and the first to probe the populations ...Rupali Chandar, Miranda Caputo, Angus Mok, Sean Linden, Bradley C. Whitmore, Paul Goudfrooij, David O. Cook, Daniela Calzetti, Debra M. Elmegreen, Janice C. Lee, Leonardo Úbeda, Richard White +11 moredoaj +1 more sourceStar-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 sourceCluster Formation in a Filamentary Cloud: The Case of the Stellar Cluster NGC 2316
The Astronomical JournalWe present a multiwavelength analysis of the star cluster NGC 2316 and its surroundings. We estimated the physical parameters of the NGC 2316 cluster, including its shape (elongated), size ( R _cluster = 0.4 pc), distance (1.3 ± 0.3 kpc), and minimum ...Saurabh Sharma, Aayushi Verma, Kshitiz Mallick, Lokesh K. Dewangan, Harmeen Kaur, Ram Kesh Yadav, Neelam Panwar, Devendra K. Ojha, Tarak Chand, Mamta Agarwal +9 moredoaj +1 more sourceEuclid: Early Release Observations – The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822★
Astronomy & AstrophysicsStar clusters are valuable indicators of galaxy evolution, offering insights into the buildup of stellar populations across cosmic time. Understanding the intrinsic star cluster populations of dwarf galaxies is particularly important given these systems’ Howell J. M., Ferguson A. M. N., Larsen S. S., Lançon A., Annibali F., Cuillandre J.-C., Hunt L. K., Martínez-Delgado D., Massari D., Saifollahi T., Voggel K., Altieri B., Andreon S., Auricchio N., Baccigalupi C., Baldi M., Bardelli S., Biviano A., Branchini E., Brescia M., Brinchmann J., Camera S., Cañas-Herrera G., Candini G. P., Capobianco V., Carbone C., Carretero J., Castellano M., Castignani G., Cavuoti S., Cimatti A., Colodro-Conde C., Congedo G., Conselice C. J., Conversi L., Copin Y., Courbin F., Courtois H. M., Cropper M., Da Silva A., Degaudenzi H., De Lucia G., Dubath F., Duncan C. A. J., Dupac X., Dusini S., Escoffier S., Farina M., Farinelli R., Faustini F., Ferriol S., Finelli F., Frailis M., Franceschi E., Fumana M., Galeotta S., George K., Gillis B., Giocoli C., Gracia-Carpio J., Grazian A., Grupp F., Haugan S. V. H., Hoekstra H., Holmes W., Hormuth F., Hornstrup A., Jahnke K., Jhabvala M., Keihänen E., Kermiche S., Kubik B., Kümmel M., Kunz M., Kurki-Suonio H., Le Brun A. M. C., Le Mignant D., Ligori S., Lilje P. B., Lindholm V., Lloro I., Mainetti G., Maino D., Maiorano E., Mansutti O., Marggraf O., Martinelli M., Martinet N., Marulli F., Massey R. J., Medinaceli E., Mei S., Melchior M., Mellier Y., Meneghetti M., Merlin E., Meylan G., Mora A., Moresco M., Moscardini L., Nakajima R., Neissner C., Niemi S.-M., Padilla C., Paltani S., Pasian F., Pedersen K., Percival W. J., Pettorino V., Pires S., Polenta G., Poncet M., Popa L. A., Raison F., Renzi A., Rhodes J., Riccio G., Romelli E., Roncarelli M., Saglia R., Sakr Z., Sapone D., Sartoris B., Schirmer M., Schneider P., Schrabback T., Secroun A., Seidel G., Serrano S., Simon P., Sirignano C., Sirri G., Skottfelt J., Stanco L., Steinwagner J., Tallada-Crespí P., Taylor A. N., Teplitz H. I., Tereno I., Toft S., Toledo-Moreo R., Torradeflot F., Tutusaus I., Valenziano L., Valiviita J., Vassallo T., Wang Y., Weller J., Zamorani G., Zinchenko I. A., Martín-Fleitas J., Scottez V. +151 moredoaj +1 more sourceDouble Star/Cluster observation of neutral sheet oscillations on 5 August 2004 [PDF]
Annales Geophysicae, 2005 Previous Cluster observations have shown that the flapping motions of the
Earth's magnetotail are of internal origin and that kink-like waves are
emitted from the central part of the tail and propagate toward the tail
flanks. The newly launched Double T. L. Zhang, T. L. Zhang, R. Nakamura, M. Volwerk, M. Volwerk, A. Runov, W. Baumjohann, H. U. Eichelberger, C. Carr, A. Balogh, V. Sergeev, J. K. Shi, K.-H. Fornacon +12 moredoaj +1 more sourceNew Wolf-Rayet star and its circumstellar nebula in Aquila
, 2009 We report the discovery of a new Wolf-Rayet star in Aquila via detection of
its circumstellar nebula (reminiscent of ring nebulae associated with late WN
stars) using the Spitzer Space Telescope archival data.A. F. Valeev, A. Y. Kniazev, Avedisova, Barniske, Benjamin, Blaauw, Blum, Bohlin, Brighenti, Carey, Chevalier, De Wit, Dehnen, Fazio, Gies, Gvaramadze, Gvaramadze, Gvaramadze, Gvaramadze, Gvaramadze, Hamann, Hamann, Hamann, Helfand, Hora, Hutsemekers, Kharchenko, Kniazev, Kniazev, Kniazev, L. N. Berdnikov, Marston, Martins, Mathis, Moffat, Moneti, Oke, Parker, Poveda, Price, Reid, Rieke, Rieke, Robberto, S. Fabrika, Schilbach, Seaton, Skrutskie, Smith, Smith, Stone, V. V. Gvaramadze, Van Der Hucht, W.-R. Hamann, Wilson, Zasov, Zinnecker +56 morecore +1 more sourceDeep Galaxy Stellar Mass Functions As a Function of Star Formation Rate in the Virgo Cluster Environment
The Astrophysical JournalWe analyze deep ( M _* ≳ 10 ^7 M _⊙ ) galaxy stellar mass functions (SMFs) of the Virgo cluster using stellar masses derived as part of the Next Generation Virgo Survey. The total SMF has a slope of $\alpha =-1.3{5}_{-0.02}^{+0.02}$ , which is similar to Cameron R. Morgan, Elizaveta Sazonova, Ian D. Roberts, Michael L. Balogh, Joel Roediger, Laura Ferrarese, Patrick Côté, Alessandro Boselli, Matteo Fossati, Jean-Charles Cuillandre, Stephen Gwyn +10 moredoaj +1 more source
