Results 31 to 40 of about 86,516 (190)

New Results on Standard Solar Models

, 2009
We describe the current status of solar modelling and focus on the problems originated with the introduction of solar abundance determinations with low CNO abundance values.
A. Weiss, Aldo M. Serenelli, B. Aharmim, B. Aharmim, C. Allende Prieto, C. Arpesella, C. Fröhlich, C.H. Lin, F. Delahaye, H.M. Antia, H.M. Antia, I.W. Roxburgh, J. Guzik, J.A. Guzik, J.C. Christensen-Dalsgaard, J.C. Christensen-Dalsgaard, J.C. Christensen-Dalsgaard, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.N. Bahcall, J.W. Ferguson, M. Asplund, M. Castro, N. Grevesse, N. Grevesse, N.R. Badnell, Q.R. Ahmad, S. Basu, S. Basu, S. Basu, S. Turck-Chiéze, W.C. Haxton, W.J. Chaplin   +37 more
core   +1 more source

HyperFLINT: Hypernetwork‐based Flow Estimation and Temporal Interpolation for Scientific Ensemble Visualization

Computer Graphics Forum, EarlyView.
Abstract We present HyperFLINT (Hypernetwork‐based FLow estimation and temporal INTerpolation), a novel deep learning‐based approach for estimating flow fields, temporally interpolating scalar fields, and facilitating parameter space exploration in spatio‐temporal scientific ensemble data. This work addresses the critical need to explicitly incorporate
Hamid Gadirov, Qi Wu, David Bauer, Kwan‐Liu Ma, Jos B.T.M. Roerdink, Steffen Frey   +5 more
wiley   +1 more source

Formation and Evolution of Planetary Systems in Presence of Highly Inclined Stellar Perturbers [PDF]

, 2011
The presence of highly eccentric extrasolar planets in binary stellar systems suggests that the Kozai effect has played an important role in shaping their dynamical architectures.
Batygin, Konstantin, Morbidelli, Alessandro, Tsiganis, Kleomenis   +2 more
core   +10 more sources

Bayesian analysis of interiors of HD 219134b, Kepler-10b, Kepler-93b, CoRoT-7b, 55 Cnc e, and HD 97658b using stellar abundance proxies [PDF]

, 2016
Using a generalized Bayesian inference method, we aim to explore the possible interior structures of six selected exoplanets for which planetary mass and radius measurements are available in addition to stellar host abundances: HD~219134b, Kepler-10b ...
Dorn, C., Hinkel, N. R., Venturini, J.
core   +2 more sources

Insights on the volcanic and impact histories of the lunar nearside from the petrology, geochemistry, and geochronology of the Calcalong Creek lunar regolith breccia meteorite

Meteoritics &Planetary Science, Volume 60, Issue 3, Page 392-421, March 2025.
Abstract The Calcalong Creek lunar meteorite is a regolith breccia with a lithologically diverse array of clasts set in a glassy, highly vesicular matrix. Here, we present a comprehensive new analysis of the meteorite. Comparisons to remote sensing data, lunar sample lithologies, and lunar sample ages indicate that it was likely sourced from regolith ...
B. H. Oliveira, J. F. Snape, R. Tartèse, J. F. Pernet‐Fisher, D. van Acken, M. J. Whitehouse, K. H. Joy   +6 more
wiley   +1 more source

Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry [PDF]

Astronomy & Astrophysics
Gravitational waves from black-hole (BH) merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected based on most stellar evolution models -- and also higher than known ...
Gaia Collaboration P. Panuzzo, T. Mazeh, F. Arenou, B. Holl, E. Caffau, A. Jorissen, C. Babusiaux, P. Gavras, J. Sahlmann, U. Bastian, L. Wyrzykowski, L. Eyer, N. Leclerc, N. Bauchet, A. Bombrun, N. Mowlavi, G. Seabroke, D. Teyssier, E. Balbinot, A. Helmi, A. Brown, A. Vallenari, T. Prusti, J. D. Bruijne, A. Barbier, M. Biermann, O. Creevey, C. Ducourant, D. Evans, R. Guerra, A. Hutton, C. Jordi, S. Klioner, U. Lammers, L. Lindegren, X. Luri, F. Mignard, C. Nicolas, S. Randich, P. Sartoretti, R. Smiljanic, P. Tanga, N. Walton, C. Aerts, C. Bailer-Jones, M. Cropper, R. Drimmel, F. Jansen, D. Katz, M. Lattanzi, C. Soubiran, F. Th'evenin, F. V. Leeuwen, R. Andrae, M. Audard, J. Bakker, R. Blomme, J. Castañeda, F. Angeli, C. Fabricius, M. Fouesneau, Y. Fr'emat, L. Galluccio, A. Guerrier, U. Heiter, E.Masana, R. Messineo, K. Nienartowicz, F. Pailler, F. Riclet, W. Roux, R. Sordo, G. Gracia-Abril, J. Portell, M. Altmann, K. Benson, J. Berthier, P. Burgess, D. Busonero, G. Busso, C. Cacciari, H. C'anovas, J. Carrasco, B. Carry, A. Cellino, N. Cheek, G. Clementini, Y. Damerdji, M. Davidson, P. D. Teodoro, L. Delchambre, A. Dell’Oro, E. F. Garcia, D. Garabato, P. Garc'ia-Lario, R. Haigron, N. Hambly, D. Harrison, D. Hatzidimitriou, J. Hern'andez, D. Hestroffer, S. Hodgkin, S. Jamal, G. D. Fombelle, S. Jordan, A. Krone-Martins, A. Lanzafame, W. Loffler, A. Lorca, O. Marchal, P. Marrese, A. Moitinho, K. Muinonen, M. N. Campos, I. Oreshina-Slezak, P. Osborne, E. Pancino, T. Pauwels, A. Recio-Blanco, M. Riello, L. Rimoldini, A. Robin, T. Roegiers, L. M. Sarro, M. Schultheis, M. Smith, A. Sozzetti, E. Utrilla, M. V. Leeuwen, K. Weingrill, U. Abbas, P. 'Abrah'am, A. Aramburu, S. Ahmed, G. Altavilla, M. A. Álvarez, F. Anders, R. I. Anderson, E. A. Varela, T. Antoja, S. Baig, D. Baines, S. Baker, L. Balaguer-N'unez, Z. Balog, C. Barache, M. Barros, M. Barstow, S. Bartolom'e, D. Bashi, J.-L. Bassilana, N. Baudeau, U. Becciani, L. Bedin, I. Bellas-Velidis, M. Bellazzini, William Beordo, M. Bernet, C. Bertolotto, S. Bertone, L. Bianchi, A. Binnenfeld, Sergi Blanco-Cuaresma, J. Bland-Hawthorn, A. Blazère, T. Boch, D. Bossini, S. Bouquillon, A. Bragaglia, J. Braine, E. Bratsolis, E. Breedt, A. Bressan, N. Brouillet, E. Brugaletta, B. Bucciarelli, A. Butkevich, R. Buzzi, A. Camut, R. Cancelliere, T. Cantat-Gaudin, D. C. Guilarte, R. Carballo, T. Carlucci, M. I. Carnerero, J. Carretero, S. Carton, L. Casamiquela, A. Casey, M. Castellani, A. Castro-Ginard, L. Ceraj, V. Cesare, P. Charlot, C. Chaudet, L. Chemin, A. Chiavassa, N. Chornay, D. Chosson, W. J. Cooper, T. Cornez, S. Cowell, M. Crosta, C. Crowley, M. C. Reyes, C. Dafonte, M. D. Ponte, M. David, P. Laverny, F. Luise, R. March, J. D. Ridder, A. Torres, E. F. D. Peloso, M. Delbo, A. Delgado, J. Delisle, C. Demouchy, E. Denis, T. Dharmawardena, F. D. Giacomo, C. Diener, E. Distefano, C. Dolding, K. Dsilva, H. Enke, C. Fabre, M. Fabrizio, S. Faigler, M. Fatovi'c, G. Fedorets, J. Fern'andez-Hern'andez, P. Fernique, F. Figueras, C. Fouron, F. Fragkoudi, M. Gai, M. Galinier, A. Garcia-Serrano, M. Garc'ia-Torres, A. Garofalo, E. Gerlach, R. Geyer, P. Giacobbe, G. Gilmore, S. Girona, G. Giuffrida, A. Gomboc, A. Gomez, I. Gonz'alez-Santamar'ia, E. Gosset, M. Granvik, V. G. Barrera, R. Guti'errez-S'anchez, M. Haywood, A. Helmer, S. L. Hidalgo, T. Hilger, D. Hobbs, C. Hottier, H. Huckle, 'O. Jim'enez-Arranz, J. Campillo, Z. Kaczmarek, P. Kervella, S. Khanna, M. Kontizas, G. Kordopatis, A. Korn, 'A. K'osp'al, Z. Kostrzewa-Rutkowska, K. Kruszy'nska, M. Kun, S. Lambert, A. Lanza, Y. Lebreton, T. Lebzelter, S. Leccia, G. Lecoutre, S. Liao, L. Liberato, E. Licata, E. Livanou, A. Lobel, J. L'opez-Miralles, C. Loup, M. Madar'asz, L. Mahy, R. G. Mann, M. Manteiga, S. Marinoni, C. Marcellino, D. J. Marshall, D. Mascarenhas, J. Marchant, J. M. Lozano, A. Masip, M. Marconi, D. Pina, L. M. Polo, J. Mart'in-Fleitas, A. Mastrobuono-Battisti, P. McMillan, J. Meichsner, J. Merc, S. Messina, N. Millar, A. Mints, D. Mohamed, D. Molina, R. Molinaro, M. Mongui'o, P. Montegriffo, L. Monti, A. Mora, R. Morbidelli, D. Morris, R. Mudimadugula, T. Muraveva, I. Musella, Z. Nagy, N. Nardetto, C. Navarrete, S. Oh, C. Ordenovic, O. Orenstein, C. Pagani, I. Pagano, L. Palaversa, P. Palicio, L. Pallas-Quintela, M. Pawlak, A. Penttila, P. Pesciullesi, M. Pinamonti, E. Plachy, L. Planquart, G. Plum, E. Poggio, D. Pourbaix, A. Price-Whelan, L. Pulone, V. Rabin, M. Rainer, C. Raiteri, P. Ramos, M. Ramos-Lerate, M. Ratajczak, P. Fiorentin, S. Regibo, C. Reyl'e, V. Ripepi, A. Riva, H. Rix, G. Rixon, G. Robert, N. Robichon, C. Robin, M. Romero-G'omez, N. Rowell, D. Mieres, K. Rybicki, G. Sadowski, A. S. Sell'es, N. Sanna, R. Santoveña, M. Sarasso, M. Sarmiento, C. S. Riera, E. Sciacca, D. S'egransan, M. Semczuk, S. Shahaf, A. Siebert, E. Slezak18, R. Smart, O. Snaith, E. Solano, F. Solitro, D. Souami, J. Souchay, E. Spitoni, F. Spoto, L. A. Squillante, I. Steele, H. Steidelmuller, J. Surdej, L. Szabados, F. Taris, M. B. Taylor, R. Teixeira, T. Tepper-García, W. Thuillot, L. Tolomei, N. Tonello, F. Torra, G. T. Elipe, M. Trabucchi, E. Trentin, M. Tsantaki, C. Turon, A. Ulla, N. Unger, I. Valtchanov, O. Vanel, A. Vecchiato, D. Vicente, E. Villar, M. Weiler, H. Zhao, J. Zorec, S. Zucker, A. vZupi'c, T. Zwitter   +413 more
semanticscholar   +1 more source

Asteroseismology of Solar-Type and Red-Giant Stars

, 2013
We are entering a golden era for stellar physics driven by satellite and telescope observations of unprecedented quality and scope. New insights on stellar evolution and stellar interiors physics are being made possible by asteroseismology, the study of ...
Chaplin, William J., Miglio, Andrea
core   +1 more source

Using X‐ray computed microtomography (μCT) to determine subsample‐specific cosmogenic noble gas production rates of E (enstatite) chondrites

Meteoritics &Planetary Science, Volume 60, Issue 3, Page 442-463, March 2025.
Abstract Cosmic ray exposure (CRE) ages provide information about the parent bodies and source regions of meteorite classes. Cosmogenic noble gases are often used to quantify exposure time scales ranging from tens of ka to hundreds of Ma. The production rate of cosmogenic noble gases is primarily controlled by a meteorite's chemical composition ...
M. Mijjum, B. J. Andrews, T. J. McCoy, C. M. Corrigan, M. W. Caffee, M. M. Tremblay   +5 more
wiley   +1 more source

The scientific potential of space-based gravitational wave detectors

, 2014
The millihertz gravitational wave band can only be accessed with a space-based interferometer, but it is one of the richest in potential sources. Observations in this band have amazing scientific potential.
A. Arvanitaki, A. Merloni, A. Petiteau, A. Sesana, A.M. Koekemoer, B.F. Schutz, C. Li, C.F. Sopuerta, C.F.B. Macedo, C.L. MacLeod, C.M. Will, D. Coe, D.J. Croton, D.J. Mortlock, E. Barausse, E. Barausse, E. Barausse, E. Bert, E. Berti, E. Berti, E. Berti, F.D. Ryan, F.D. Ryan, G. Hobbs, G. Nelemans, J.E. Greene, J.R. Gair, J.R. Gair, J.R. Gair, J.R. Gair, K. Danzmann, K. Glampedakis, K. Yagi, K.G. Arun, K.G. Arun, K.G. Arun, L. Barack, L. Barack, M. Kesden, M. Tinto, N. Cornish, N. Yunes, N. Yunes, N. Yunes, N.A. Collins, N.A. Grogin, P. Amaro-Seoane, P. Amaro-Seoane, P. Amaro-Seoane, P. Amaro-Seoane, P. Binetruy, P. Canizares, P. Pani, P.A.R. Ade, R.K. Sheth, S. Gossan, S. Hilbert, S. Nissanke, S. Tremaine, S. Vigeland, S.A. Hughes, S.W. Hawking, T.A. Apostolatos   +62 more
core   +1 more source

A primitive asteroid that lived fast and died young sampled by a xenolith in the Cold Bokkeveld CM2 carbonaceous chondrite

Meteoritics &Planetary Science, Volume 60, Issue 3, Page 464-483, March 2025.
Abstract Xenoliths in carbonaceous chondrites include lithologies that are unrepresented in the meteorite record and so are a rich source of information on asteroid diversity. Cold Bokkeveld is a CM2 regolith breccia that contains both hydrous and anhydrous lithic clasts. Here, we describe a hydrous clast with a fine‐grained rim.
Martin R. Lee, Cameron J. Floyd, Robin Haller, Sammy Griffin   +3 more
wiley   +1 more source