Zobrazeno 1 - 10
of 179
pro vyhledávání: '"Ewald Müller"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 486:2238-2253
We present predictions for the gravitational-wave (GW) emission of three-dimensional supernova (SN) simulations performed for a 15 solar-mass progenitor with the Prometheus-Vertex code using energy-dependent, three-flavor neutrino transport. The prog
Publikováno v:
EAS Publications Series
Jean-Paul Zahn’s formalism for vertical shear mixing is used in several stellar evolution codes, but the physics of the shear instability in stellar radiative zones is still not completely understood. Over the last few years, numerical simulations
Autor:
Alexander Heger, T. Ertl, H.-Th. Janka, A. Menon, Annop Wongwathanarat, V. P. Utrobin, Ewald Müller
Six binary-merger progenitors of Supernova 1987A (SN 1987A) with properties close to those of the blue supergiant Sanduleak -69 202 are exploded by neutrino heating and evolved until long after shock breakout in three dimensions (3D), and continued f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b3b59507b5c3ce5918c55d712b01e0a6
http://arxiv.org/abs/2102.09686
http://arxiv.org/abs/2102.09686
The extent of mixed regions around convective zones is one of the biggest uncertainties in stellar evolution. 1D overshooting descriptions introduce a free parameter ($f_{ov}$) that is in general not well constrained from observations. Especially in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::caf93b96fe544ae3e7a5dd8e44204114
http://arxiv.org/abs/2012.05262
http://arxiv.org/abs/2012.05262
Autor:
Karen Haase, Wolfgang Schmidt, Oliviero De Simone, Wolfgang J. Junk, Guido Gonsior, Ewald Müller
Publikováno v:
Functional plant biology : FPB. 29(9)
Adaptation to prolonged flooding was investigated using cuttings of two tree species from the Central Amazon white-water floodplain (V�rzea). Morphological features and oxygen distribution patterns were correlated with metabolic changes under hypox
Autor:
Pedro J. Montero, Ewald Müller, Niccolò Bucciantini, L. Del Zanna, Jérôme Guilet, Matteo Bugli
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Monthly Notices of the Royal Astronomical Society, 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Mon.Not.Roy.Astron.Soc., 2018, 475, pp.108. 〈10.1093/mnras/stx3158〉
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Monthly Notices of the Royal Astronomical Society, 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 475 (1), pp.108-120. ⟨10.1093/mnras/stx3158⟩
Mon.Not.Roy.Astron.Soc., 2018, 475, pp.108. 〈10.1093/mnras/stx3158〉
Geometrically thick tori with constant specific angular momentum have been widely used in the last decades to construct numerical models of accretion flows onto black holes. Such discs are prone to a global non-axisymmetric hydrodynamic instability,
Autor:
Alexei Mate, Pablo Cerdá-Durán, Nikolaos Stergioulas, José A. Font, Michael Gabler, Ewald Müller
Publikováno v:
Astronomische Nachrichten. 338:1105-1108
Magneto-elastic oscillations of neutron stars are believed to explain observed quasi-periodic oscillations (QPOs) in the decaying tail of the giant flares of highly magnetized neutron stars (magnetars). Strong efforts of the theoretical modelling fro
Cassiopeia A, one of the most intriguing galactic supernova remnants, has been a target of many observational efforts including most recent observations by ALMA, Hubble, Herschel, Spitzer, NuSTAR, Integral, and other observatories. We use recent gamm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dec31d32b16425bc4bd5a2019457f842
We present a new method for solving the three-dimensional gravitational potential of a density field on the Yin-Yang grid. Our algorithm is based on a multipole decomposition and completely symmetric with respect to the two Yin-Yang grid patches. It
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b375c46253b8cd82e2e8703fdd2d002f
http://arxiv.org/abs/1806.04593
http://arxiv.org/abs/1806.04593
Autor:
S. Kellner, Pierre Kervella, Faustine Cantalloube, Johana Panduro, Magdalena Lippa, V. Coudé du Foresto, Y. Clénet, R. Abuter, G. Avila, Matteo Accardo, Konrad R. W. Tristram, Dan Popovic, Alejandra Rosales, A. Buron, R. Genzel, C. Deen, Laurent Jocou, Markus Schöller, T. Ott, H. Bonnet, P. Fédou, Frank Eisenhauer, R. van Boekel, Stefan Hippler, André Müller, Pierre Léna, Thibaut Moulin, Julien Woillez, L. Pallanca, Ekkehard Wieprecht, P.-O. Petrucci, N. Hubin, Leander Mehrgan, Sylvestre Lacour, Markus Wittkowski, Vincent Lapeyrere, Christian A. Hummel, M. Haug, Eckhard Sturm, Frederic Derie, Thanh Phan Duc, Sarah Kendrew, Burkhard Wolff, Mario Kiekebusch, Nicolas Blind, Andreas Kaufer, W. J. de Wit, Feng Gao, C. Collin, Silvia Scheithauer, L. Kern, Roderick Dembet, Matthew Horrobin, J.-U. Pott, Stefan Gillessen, Johann Kolb, Narsireddy Anugu, R.-R. Rohloff, M. Riquelme, J. Sanchez-Bermudez, Andreas Eckart, J. Moreno-Ventas, R. Brast, Z. Hubert, Isabelle Percheron, M. Mellein, F. Delplancke-Ströbele, M. Karl, Udo Neumann, Imke Wank, Rainer Lenzen, Odele Straub, Michael Esselborn, Armin Huber, J.-B. Le Bouquin, Ralf Klein, Juan-Luis Ramos, Erich Wiezorrek, Samuel Lévêque, K. Perraut, Frédéric Cassaing, C. E. Garcia Dabo, F. Müller, P. M. Plewa, Ewald Müller, N. Ventura, F. Chapron, Gerd Weigelt, M. Ebert, Martin Kulas, M. Wiest, Elodie Choquet, Luca Pasquini, A. Caratti o Garatti, A. Pflüger, T. de Zeeuw, Guy Perrin, Myriam Benisty, Yves Magnard, Joachim M. Bestenlehner, S. Oberti, António Amorim, Nicolas Schuhler, B. Lazareff, Paulo J. V. Garcia, Jason Dexter, Christian Straubmeier, Th. Henning, Jason Spyromilio, F. H. Vincent, A. Mérand, Senol Yazici, Felix Widmann, C. Rau, Pierre Bourget, R. J. García López, Xavier Haubois, Eric Gendron, Gérard Zins, G. Rousset, Andres J. Ramirez, Gilles Duvert, T. Paumard, Lieselotte Jochum, Idel Waisberg, F. Haussmann, O. Pfuhl, Sebastian Rabien, G. Rodríguez-Coira, Gerd Jakob, J. P. Berger, Wolfgang Brandner, D. Ziegler, Marcos Suarez
Publikováno v:
Astronomy and Astrophysics, 618, A125
Context. η Car is one of the most intriguing luminous blue variables in the Galaxy. Observations and models of the X-ray, ultraviolet, optical, and infrared emission suggest a central binary in a highly eccentric orbit with a 5.54 yr period residing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dbf1026b460a873ee87272f7110219dd
http://hdl.handle.net/1887/70609
http://hdl.handle.net/1887/70609