Results 11 to 20 of about 386,815 (325)
The Protostellar Luminosity Function [PDF]
The Astrophysical Journal, 2011 The protostellar luminosity function (PLF) is the present-day luminosity
function of the protostars in a region of star formation. It is determined
using the protostellar mass function (PMF) in combination with a stellar
evolutionary model that provides ...Andre, Baraffe, Bonnell, Christopher F. McKee, Connelley, Covey, Dunham, Dunham, Enoch, Enoch, Evans, Fuchs, Greene, Hartmann, Heiderman, Hosokawa, Hosokawa, Kirk, Kratter, Masunaga, McKee, McKee, McKee, McLaughlin, Mellon, Miller, Muzerolle, Myers, Myers, Offner, Offner, Offner, Palla, Pech, Robitaille, Sandell, Stella S. R. Offner, Tan, Vorobyov, White, White, Whitney, Young, Zhu +43 morecore +3 more sourcesRemarks on the maximum luminosity [PDF]
Physical Review D, 2018 The quest for fundamental limitations on physical processes is old and
venerable. Here, we investigate the maximum possible power, or luminosity, that
any event can produce.Cardoso, Vitor, Ikeda, Taishi, Moore, Christopher J., Yoo, Chul-Moon +3 morecore +2 more sourcesLuminosity by Attrition [PDF]
Nature, 1920 WITH reference to Sir Ray Lankester's suggestion in NATURE of November 4 that chemists should endeavour to ascertain the cause of the “empyreumatic” odour which accompanies the flashes of light produced by rubbing two quartz pebbles together, may I suggest also that the inquiry might be extended to include other substances which possess this property ... +17 more sourcesThe nuclear to host galaxy relation of high redshift quasars [PDF]
, 2007 We present near-infrared imaging with ESO VLT+ISAAC of the host galaxies of
low luminosity quasars in the redshift range 1 < z < 2, aimed at investigating
the relationship between the nuclear and host galaxy luminosities at high
redshift.Aldo Treves, Bower R. G., Dunlop J. S., Francis P. J., Jari K. Kotilainen, Kormendy J., Kotilainen J. K., Marzia Labita, Michela Uslenghi, Renato Falomo, Taylor G. L. +10 morecore +3 more sourcesPrecision luminosity measurements at LHCb [PDF]
Journal of Instrumentation, 2014 100 pages, 57 ...C. Santamarina Rios, S. Farry, A. Satta, Thomas Blake, Biagio Saitta, Hans Dijkstra, Jing Wang, P. Vazquez Regueiro, M. T. Tran, M. Sirendi, M. Stahl, O. Aquines Gutierrez, Robert Appleby, A. Pistone, Ivan Belyaev, S. Roiser, B. K. Pal, R. Silva Coutinho, R. Märki, A. Bien, F. Maciuc, P. Henrard, E. Pesen, G. Raven, Francesco Dettori, Markus Frank, Sai-Juan Chen, A. Leflat, L. A. Granado Cardoso, Maurizio Martinelli, M. Deckenhoff, P. M. Bjørnstad, Valery Pugatch, Michal Kreps, S. Tolk, F. Teubert, C. Langenbruch, R. Andreassen, D. M. Saunders, Alexander Malinin, A. Massafferri, E. Ben-Haim, Tomasz Fiutowski, G. Martellotti, Sarah Karodia, D. Websdale, Lucio Anderlini, Lucio Anderlini, M. De Cian, B. Muster, J. Maratas, P. Owen, Xavier Vilasis-Cardona, G. Mancinelli, L. Henry, B. Hamilton, R. Nandakumar, N. Farley, Rudolf Oldeman, J. Serrano, Michael Kolpin, N. Déléage, I. Raniuk, L. Cojocariu, V. Egorychev, A. Palano, B. Gui, Olivier Leroy, M. Kucharczyk, I. V. Machikhiliyan, V. Obraztsov, G. A. Cowan, D. Vieira, Luca Tomassetti, Vladimir Gligorov, P. Griffith, Dmitry Golubkov, J. P. Lees, Yang Li, B. Couturier, H. Luo, A. Oyanguren, Martino Borsato, Stefano Gallorini, F. Machefert, Adam Benjamin Morris, D. Souza, P. Szczypka, K. Müller, Mauro Morandin, D. Hill, V. Kudryavtsev, G. Valenti, D. Wiedner, Fergus Wilson, A. Gallas Torreira, Julien Cogan, Marianna Fontana, R. Calabrese, J. Bressieux, S. Kandybei, M. Liles, Konstantinos Petridis, N. Hussain, K. De Bruyn, Kurt Rinnert, Z. Xing, M. Witek, P. Naik, C. J. Parkinson, F. Dupertuis, M. Gandelman, P. Sail, Miroslaw Firlej, J. Panman, M. H. Schune, Lars Eklund, V. Battista, Hal Evans, N. A. Smith, Lluis Garrido, Alexey Badalov, F. Kruse, L. Carson, L. Castillo Garcia, O. Stenyakin, M. Fiore, I. Komarov, E. Tournefier, J. Jalocha, W. Wislicki, William Barter, C. Parkes, F. Martinez Vidal, J. M. Otalora Goicochea, R. Gauld, Bernardo Adeva, P. Rodriguez Perez, J. Prisciandaro, S. Ogilvy, J. Wicht, M. Smith, U. Straumann, Jinlin Fu, E. van Herwijnen, S. Topp-Joergensen, D. Hynds, G. Collazuol, A. Romero Vidal, A. Grecu, Marco Adinolfi, M. Korolev, A. Zvyagin, B. Spaan, P. Perret, R. Mountain, A. Hicheur, M. Orlandea, D. Savrina, W. Sutcliffe, D. A. Milanes, C. Marin Benito, Wander Baldini, M. Patel, R. Cenci, P. Gandini, Roel Aaij, U. Uwer, E. Gushchin, S. Blusk, R. Matev, G. Veneziano, G. Graziani, Luciano Pappalardo, Alessio Sarti, O. Okhrimenko, Matthew Kelsey, A. Golutvin, P. E. L. Clarke, Bo Liu, T. Skwarnicki, Krzysztof Swientek, B. Storaci, Nicola Neri, G. Lanfranchi, Stephan Eisenhardt, Jakub Moron, Alexander Bondar, Colin Barschel, M. Schmelling, A. Sparkes, O. Steinkamp, S. Playfer, Jonas Rademacker, F. Jing, H. Schindler, T. Lesiak, S. Filippov, J. H. Lopes, N. Lopez-March, F. J. P. Soler, E. Gersabeck, A. Trisovic, A. Puig Navarro, R. Stroili, K. Belous, A. McNab, George Lafferty, D. Dossett, Gianluigi Casse, M. Hoballah, A. Sciubba, Nicola Serra, A. Dzyuba, A. Ustyuzhanin, D. Tonelli, Y. Zhang, Manuel Schiller, M. Cruz Torres, Thomas Latham, F. Palombo, M. Veltri, Massimiliano Fiorini, C. Bozzi, C. Prouve, A. Mapelli, Claudio Gotti, Michael Alexander, A. Lai, E. Smith, O. Lupton, Gabriele Simi, S. Perazzini, C. J. G. Onderwater, Eleonora Luppi, M. Schubiger, V. Fernandez Albor, J. Molina Rodriguez, I. Nasteva, Lorenzo Sestini, L. De Paula, F. Blanc, Themistocles Bowcock, V. Niess, M. Zavertyaev, A. Contu, Patrick Koppenburg, Marta Calvi, Johannes Albrecht, Marcello Rotondo, C. Vázquez Sierra, Angelo Geraci, Anton Poluektov, P. Seyfert, M. Dorigo, N. K. Watson, Barbara Sciascia, A. Di Canto, M. J. Morello, J. García Pardiñas, M. S. Rangel, J. J. Saborido Silva, S. Cadeddu, K. Carvalho Akiba, R. Santacesaria, C. Potterat, F. Bedeschi, J. D. Price, J. van Tilburg, E. Rodrigues, S. De Capua, C. Satriano, X. Cid Vidal, O. Schneider, R. Le Gac, Christoph Frei, Giulio Dujany, Marina Artuso, Alessandro Cardini, P. Alvarez Cartelle, S. Klaver, Roberta Cardinale, A. Ukleja, R. Vazquez Gomez, A. A. Alves, R. Lefèvre, D. Gascon, W. Bonivento, S. Vecchi, N. H. Brook, R. Graciani Diaz, A. Dziurda, S. Benson, S. Coquereau, Philip Ilten, A. Tsaregorodtsev, D. Martinez Santos, G. Punzi, F. Redi, C. Patrignani, C. Matteuzzi, Giovanni Carboni, I. Shapoval, P. Krokovny, F. Dordei, David Hutchcroft, Marek Idzik, M. Calvo Gomez, G. Pessina, Pieter David, A. Gianelle, Tomasz Szumlak, S. Stracka, P. Marino, Jolanta Brodzicka, M. Vieites Diaz, B. Popovici, V. Tisserand, Victor Coco, Roger Barlow, J. A. Hernando Morata, Simone Bifani, Zhenwei Yang, A. Petrolini, D. Galli, C. Farinelli, M. Perrin-Terrin, S. Esen, S. Cunliffe, G. Passaleva, Sheldon Stone, M. Needham, E. Cogneras, F. Ferreira Rodrigues, E. Picatoste Olloqui, F. Archilli, G. Manca, A. Lupato, Marco Cattaneo, Manuel Mussini, E. Santovetti, Ulrik Egede, C. Fitzpatrick, G. Corti, J. A. de Vries, Olivier Deschamps, C. Lazzeroni, J. Dalseno +347 moreopenaire +20 more sourcesThe Luminosity Determination [PDF]
Highlights of Astronomy, 1995 The Hertzprung-Russel (HR) diagram luminosity calibration relies basically on three kinds of data: trigonometric parallaxes, kinematical data (proper motions and radial velocities) and cluster distances obtained by the zero-age main sequence fitting procedure.C. Turon, A.E. Gómezopenaire +1 more source
