Zobrazeno 1 - 10
of 53
pro vyhledávání: '"Burkhard Wolff"'
Autor:
Christian Straubmeier, Oliver Pfuhl, Elodie Choquet, Wolfgang Brandner, Xavier Haubois, P. Fédou, Roderick Dembet, Sylvestre Lacour, Guy Perrin, Burkhard Wolff, Julien Woillez, Karine Perraut, A. Ramirez, António Amorim, Konrad R. W. Tristram, Ekkehard Wieprecht, Roberto Abuter, Frédéric Cassaing, T. Ott, Erich Wiezorrek, Frank Eisenhauer
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 624, pp.A99. ⟨10.1051/0004-6361/201834981⟩
Astronomy and Astrophysics
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2019, 624, pp.A99. ⟨10.1051/0004-6361/201834981⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 624, pp.A99. ⟨10.1051/0004-6361/201834981⟩
Astronomy and Astrophysics
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2019, 624, pp.A99. ⟨10.1051/0004-6361/201834981⟩
The GRAVITY instrument has been commissioned on the VLTI during 2016 and is now available to the astronomical community. It is the first optical interferometer capable of observing sources as faint as magnitude 19 in K-band. This is possible thanks t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::abb6987d13e15a73010127f0ba42aecf
https://hal.sorbonne-universite.fr/hal-02113844/file/aa34981-18.pdf
https://hal.sorbonne-universite.fr/hal-02113844/file/aa34981-18.pdf
Autor:
Roderick Dembet, Sylvestre Lacour, Burkhard Wolff, Karine Rousselet-Perraut, Christian Straubmeier, Frank Eisenhauer, António Amorim, Vincent Lapeyrere, Wolfgang Brandner, Jean-Baptiste Le Bouquin, Guy Perrin, Xavier Haubois
Publikováno v:
Optical and Infrared Interferometry and Imaging VI.
The GRAVITY instrument installed at VLTI uses differential fibered delay lines to spatially filter the incoming wavefronts and accurately control the optical path difference between the Fringe Tracker (FT) and Scientific Detector (SC) parts of the in
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
Autor:
Christian A. Hummel, J. Taylor, Daniel Asmus, Hans-Ulrich Käufl, Florian Kerber, J. Vinther, Konrad R. W. Tristram, Burkhard Wolff, Alain Smette, Mario van den Ancker
Publikováno v:
Observatory Operations: Strategies, Processes, and Systems VI.
A comparison of the FWHM of standard stars observed with VISIR, the mid-IR imager and spectrometer at ESO's VLT, with expectations for the achieved mid-IR Image Quality based on the optical seeing and the wavelength-dependence of atmospheric turbulen
Autor:
Beate Stelzer, R. V. Yudin, Zdeněk Mikulášek, Swetlana Hubrig, Burkhard Wolff, Ilya Ilyin, M. A. Pogodin, Markus Schöller, Charles R. Cowley
Publikováno v:
Astronomische Nachrichten. 332:1022-1026
New determinations of the mean longitudinal magnetic field for several Herbig Ae/Be stars are presented. The longitudinal magnetic field measurements of MWC 480 reveal the presence of a strong kG field, which was undetected in our previous low-resolu
Publikováno v:
Astronomy & Astrophysics. 489:315-320
Aims. Our goal is to measure the nitrogen abundance in 5 turn off (TO) stars of the two globular clusters NGC 6397 and NGC 6752, and to compare the cluster abundances with those of field stars of comparable metallicity. In addition, we investigate th
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 377:1579-1587
Large wavelength shifts of infrared triplet lines of Ca II have been observed in the spectra of HgMn and magnetic Ap stars. They have been attributed to the heavy calcium isotopes, including Ca-48. One member of the triplet, $\lambda$8542, had been e
Autor:
V. G. Elkin, D. W. Kurtz, Swetlana Hubrig, Margarida S. Cunha, Gautier Mathys, I. S. Savanov, Burkhard Wolff
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 372:286-292
HD154708 has an extraordinarily strong magnetic field of 24.5kG. Using 2.5h of high timeresolution Ultraviolet and Visual Echelle Spectrograph (UVES) spectra we have discoveredthis star to be an roAp star with a pulsation period of 8min. The radial
Autor:
Margarida S. Cunha, Gautier Mathys, Pierre North, Nicole Nesvacil, Swetlana Hubrig, D. W. Kurtz, Markus Schöller, Burkhard Wolff, V. G. Elkin, Thomas Szeifert
Publikováno v:
Astronomy & Astrophysics. 440:L37-L40
We have discovered an extraordinarily large mean longitudinal magnetic field of 7.5 kG in the ultra-cool low mass Ap star HD 154708 using FORS 1 in spectropolarimetric mode. From UVES spectra, we have measured a mean magnetic field modulus of 24.5 kG
This book constitutes the refereed proceedings of the 4th International Symposium on Unifying Theories of Programming, UTP 2012, held in Paris, France, in August 2012, co-located with the 18th International Symposium on Formal Methods, FM 2012. The 8