Zobrazeno 1 - 10
of 200
pro vyhledávání: '"D. Schertl"'
Autor:
J. W. Isbell, K. Meisenheimer, J.-U. Pott, M. Stalevski, K. R. W. Tristram, J. Sanchez-Bermudez, K.-H. Hofmann, V. Gámez Rosas, W. Jaffe, L. Burtscher, J. Leftley, R. Petrov, B. Lopez, T. Henning, G. Weigelt, F. Allouche, P. Berio, F. Bettonvil, P. Cruzalebes, C. Dominik, M. Heininger, M. Hogerheijde, S. Lagarde, M. Lehmitz, A. Matter, A. Meilland, F. Millour, S. Robbe-Dubois, D. Schertl, R. van Boekel, J. Varga, J. Woillez
Publikováno v:
Astronomy & Astrophysics, 663:A35. EDP Sciences
Astronomy & Astrophysics, 663, A35
Astronomy & Astrophysics, 663, A35
Active galactic nuclei play a key role in the evolution of galaxies, but their inner workings and physical connection to the host are poorly understood due to a lack of angular resolution. Infrared interferometry makes it possible to resolve the circ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d35d7bb0bcf778e80898e9ae52f9ef1
Autor:
J. Drevon, F. Millour, P. Cruzalèbes, C. Paladini, J. Hron, A. Meilland, F. Allouche, B. Aringer, P. Berio, W.C. Danchi, V. Hocdé, K.-H. Hofmann, S. Lagarde, B. Lopez, A. Matter, R. Petrov, S. Robbe-Dubois, D. Schertl, P. Stee, F. Vakili, J. Varga, R. Waters, G. Weigelt, J. Woillez, M. Wittkowski, G. Zins
Publikováno v:
Proceedings of the International Astronomical Union, 16(S366), 190-195
Proceedings of the International Astronomical Union, 16, S366, pp. 190-195
Proceedings of the International Astronomical Union, 16, 190-195
Proceedings of the International Astronomical Union, 16, S366, pp. 190-195
Proceedings of the International Astronomical Union, 16, 190-195
Carbon-rich dust is known to form in the atmosphere of the semiregular variable star R Sculptoris. Such stardust, as well as the molecules and gas produced during the lifetime of the star, will be spread into the Galaxy via the mass-loss process. Pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::685be177dc82965ba81b5811eadf8ad8
http://hdl.handle.net/1887/3515606
http://hdl.handle.net/1887/3515606
Akademický článek
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Autor:
F. Lykou, P. Ábrahám, L. Chen, J. Varga, Á. Kóspál, A. Matter, M. Siwak, Zs. M. Szabó, Z. Zhu, H. B. Liu, B. Lopez, F. Allouche, J.-C. Augereau, P. Berio, P. Cruzalèbes, C. Dominik, Th. Henning, K.-H. Hofmann, M. Hogerheijde, W. J. Jaffe, E. Kokoulina, S. Lagarde, A. Meilland, F. Millour, E. Pantin, R. Petrov, S. Robbe-Dubois, D. Schertl, M. Scheuck, R. van Boekel, L. B. F. M. Waters, G. Weigelt, S. Wolf
Publikováno v:
Astronomy & Astrophysics, 663:A86
Astronomy & Astrophysics, 663:A86. EDP Sciences
Astronomy & Astrophysics, 663, pp. 1-17
Astronomy & Astrophysics, 663, 1-17
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142788⟩
Astronomy & Astrophysics
Astronomy & Astrophysics, 663:A86. EDP Sciences
Astronomy & Astrophysics, 663, pp. 1-17
Astronomy & Astrophysics, 663, 1-17
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142788⟩
Astronomy & Astrophysics
The disk of FU Orionis is marginally resolved with MATISSE, suggesting that the region emitting in the thermal infrared is rather compact. An upper limit of $\sim1.3\pm0.1$ mas (in $L$) can be given for the diameter of the disk region probed in the $
Autor:
William C. Danchi, Luca Pasquini, Lars Venema, Leonard Burtscher, Josef Hron, Markus Wittkowski, J. Beltran, H. Méheut, Antoine Mérand, Sylvie Robbe-Dubois, A. Jaskó, Th. Henning, Farrokh Vakili, F. Guitton, Anthony Meilland, J. Vinther, Carsten Dominik, A. Gabasch, S. Rousseau, E. Kokoulina, M. Ebert, P. Antonelli, J.-U. Pott, N. Tromp, J.-L. Lizon, F. Rigal, J. Kragt, Markus Schöller, Ronald Roelfsema, Romain Petrov, L. Klarmann, P. Guajardo, Karl Heinz Hofmann, R. Frahm, Klaus Meisenheimer, Alexis Matter, F. Wrhel, Nicolas Schuhler, Gerd Jakob, Gerd Weigelt, Ph. Stee, Laurent Pallanca, A. Marcotto, Pierre Cruzalèbes, A. Chelli, I. Percheron, J. C. González Herrera, Andreas Glindemann, Claudia Paladini, Jean-Michel Clausse, M. de Haan, Eddy Elswijk, K. Meixner, Felix Bettonvil, S. Morel, R. Castillo, Uwe Graser, E. Nußbaum, Paul Bristow, Péter Ábrahám, J. W. Isbell, Eric Pantin, T. Maurer, R. ter Horst, Bruno Lopez, R. van Boekel, T. Adler, A. van Duin, L. Mosoni, Alexandre Gallenne, Udo Neumann, Ralf Conzelmann, Jean-Charles Augereau, Yves Bresson, Ramón Navarro, Norbert Hubin, M. Accardo, E. Garces, F. Allouche, Julien Woillez, Th. Rivinius, Y. Fantei, S. Abadie, A. Ridinger, Derek Ives, F. Donnan, G. Bazin, Ralf Klein, Udo Beckmann, M. Mellein, Roberto Abuter, Eszter Pozna, Sebastian Wolf, Tibor Agócs, J. Meisner, D. Schertl, L. Mohr, Marcelo Lopez, L. Jochum, Ralf-Rainer Rohloff, C. Connot, A. Soulain, Claudia Cid, W. Laun, C. Stephan, M. Heininger, R. Brast, V. Gámez Rosas, W. Boland, Michiel R. Hogerheijde, Ph. Berio, Marco Delbo, Christoph Leinert, S. Kuindersma, L. Labadie, A. Böhm, Xavier Haubois, N. Mauclert, Leander Mehrgan, F. Y. J. Gonté, M. Schuil, L. B. F. M. Waters, G. Zins, P. Bourget, R. S. Le Poole, P. Girard, M. Riquelme, József Varga, Florentin Millour, Stephane Lagarde, Walter Jaffe, R. Huerta, M. Lehmitz, G. Kroes, G. Yoffe, C. Bailet
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 647, pp.A56. ⟨10.1051/0004-6361/202039400⟩
Astronomy & Astrophysics, 647
Astronomy & Astrophysics
Astronomy & Astrophysics, 647, 1-22
HAL
Astronomy & Astrophysics, 647:A56. EDP Sciences
Astronomy and Astrophysics-A&A, EDP Sciences, In press
Astronomy & Astrophysics, 647, pp. 1-22
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 647, pp.A56. ⟨10.1051/0004-6361/202039400⟩
Astronomy & Astrophysics, 647
Astronomy & Astrophysics
Astronomy & Astrophysics, 647, 1-22
HAL
Astronomy & Astrophysics, 647:A56. EDP Sciences
Astronomy and Astrophysics-A&A, EDP Sciences, In press
Astronomy & Astrophysics, 647, pp. 1-22
Context. The inner few au region of planet-forming disks is a complex environment. High angular resolution observations have a key role in understanding the disk structure and the dynamical processes at work. Aims. In this study we aim to characteriz
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::467758444646be7bd9c76a1d04826dfe
https://hal.archives-ouvertes.fr/hal-03320683
https://hal.archives-ouvertes.fr/hal-03320683
Autor:
M. Schuil, G. Zins, Y. Fantei, Udo Beckmann, Péter Ábrahám, Anthony Meilland, K. Shabun, Philippe Stee, Farrokh Vakili, Ronald Roelfsema, A. Böhm, Andrea Chiavassa, G. Niccolini, L. Labadie, L. Mosoni, M. Riquelme, Alexandre Gallenne, P. Antonelli, R. Frahm, J.-L. Lizon, Markus Schöller, Ralf-Rainer Rohloff, Florentin Millour, Jean-Michel Clausse, Udo Neumann, F. Wrhel, M. de Haan, J. Meisner, Leonard Burtscher, R. Huerta, F. Allouche, Luca Pasquini, E. Garces, Pierre Cruzalèbes, Nicolas Nardetto, S. Morel, Behnam Javanmardi, P. Bourget, L. Jochum, A. Ridinger, R. S. Le Poole, Th. Rivinius, Bruno Lopez, V. Hocdé, Marco Delbo, I. Percheron, P. Girard, J. C. González Herrera, M. Accardo, G. Bazin, Karl Heinz Hofmann, Laszlo Szabados, J. W. Isbell, Eric Pantin, Jaime Alonso, Josef Hron, D. Schertl, Eszter Pozna, L. Klarmann, Th. Henning, S. Rousseau, C. Connot, E. Nußbaum, Eddy Elswijk, Louise Breuval, Antoine Mérand, R. van Boekel, E. Kokoulina, Leander Mehrgan, József Varga, Roberto Abuter, Markus Wittkowski, T. Adler, E. Lagadec, Claudia Paladini, M. Heininger, F. Guitton, Nicolas Schuhler, W. Laun, Romain Petrov, A. Jaskó, S. Abadie, R. ter Horst, Stephane Lagarde, R. Brast, F. Y. J. Gonté, Norbert Hubin, William C. Danchi, V. Gámez Rosas, A. Soulain, Walter Jaffe, Pierre Kervella, W. Boland, Ramón Navarro, Michiel R. Hogerheijde, Julien Woillez, K. Meixner, Felix Bettonvil, S. Borgniet, J. Beltran, Uwe Graser, Ph. Berio, Ralf Klein, J. Idserda, M. Lopez, Klaus Meisenheimer, Andreas Glindemann, J.-U. Pott, H. Hanenburg, Lars Venema, Sylvie Robbe-Dubois, Alexis Matter, Tibor Agócs, R. Buter, M. Ebert, Carsten Dominik, P. Guajardo, Laurent Pallanca, A. Marcotto, R. Waters, A. Gabasch, R. Castillo, M. Lehmitz, Jean-Charles Augereau, Derek Ives, Yves Bresson, S. Kuindersma, A. Glazenborg, Claudia Cid, C. Stephan, Sebastian Wolf, L. Mohr, J. Kragt, Christoph Leinert, F. Rigal, N. Tromp, Xavier Haubois, N. Mauclert, Gerd Jakob, Gerd Weigelt, J. Vinther, A. Chelli, C. Bailet, Paul Bristow, A. Domiciano de Souza, T. Maurer, A. van Duin, Ralf Conzelmann, M. Mellein, G. Kroes, G. Yoffe, T. Phan Duc
Publikováno v:
Astronomy & Astrophysics, 651, 1-13
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 651, pp.A92. ⟨10.1051/0004-6361/202140626⟩
Astronomy & Astrophysics, 651, pp. 1-13
Astronomy & Astrophysics, 651:A92. EDP Sciences
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 651, pp.A92. ⟨10.1051/0004-6361/202140626⟩
Astronomy & Astrophysics, 651, pp. 1-13
Astronomy & Astrophysics, 651:A92. EDP Sciences
The nature of circumstellar envelopes (CSE) around Cepheids is still a matter of debate. The physical origin of their infrared (IR) excess could be either a shell of ionized gas, or a dust envelope, or both. This study aims at constraining the geomet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a89dfc3e8511451152a1ed03b61ae405
https://doi.org/10.1051/0004-6361/202140626
https://doi.org/10.1051/0004-6361/202140626
VLTI-MATISSE L- and N-band aperture-synthesis imaging of the unclassified B[e] star FS Canis Majoris
Autor:
K.-H. Hofmann, A. Bensberg, D. Schertl, G. Weigelt, S. Wolf, A. Meilland, F. Millour, L. B. F. M. Waters, S. Kraus, K. Ohnaka, B. Lopez, R. G. Petrov, S. Lagarde, Ph. Berio, F. Allouche, S. Robbe-Dubois, W. Jaffe, Th. Henning, C. Paladini, M. Schöller, A. Mérand, A. Glindemann, U. Beckmann, M. Heininger, F. Bettonvil, G. Zins, J. Woillez, P. Bristow, P. Stee, F. Vakili, R. van Boekel, M. R. Hogerheijde, C. Dominik, J.-C. Augereau, A. Matter, J. Hron, E. Pantin, Th. Rivinius, W.-J. de Wit, J. Varga, L. Klarmann, K. Meisenheimer, V. Gámez Rosas, L. Burtscher, J. Leftley, J. W. Isbell, G. Yoffe, E. Kokoulina, W. C. Danchi, P. Cruzalèbes, A. Domiciano de Souza, J. Drevon, V. Hocdé, A. Kreplin, L. Labadie, C. Connot, E. Nußbaum, M. Lehmitz, P. Antonelli, U. Graser, C. Leinert
Publikováno v:
Astronomy & Astrophysics, 658, pp. 1-25
Astronomy & Astrophysics, 658, 1-25
Astronomy and Astrophysics, 658:A81. EDP Sciences
Astronomy & Astrophysics, 658:A81
Astronomy & Astrophysics, 658, 1-25
Astronomy and Astrophysics, 658:A81. EDP Sciences
Astronomy & Astrophysics, 658:A81
Context: FS Canis Majoris (FS CMa, HD 45677) is an unclassified B[e] star surrounded by an inclined dust disk. The evolutionary stage of FS CMa is still debated. Perpendicular to the circumstellar disk, a bipolar outflow was detected. Infrared apertu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2864d53187c767aa14e7a8ef33c15f55
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
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K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
M. Heininger, R. van Boekel, Sebastian Wolf, Gerd Weigelt, Romain Petrov, Ph. Berio, Josef Hron, Paul Bristow, Anthony Meilland, Eric Pantin, S. Morel, G. Kroes, Bruno Lopez, Florentin Millour, Felix Bettonvil, Sylvie Robbe-Dubois, Klaus Meisenheimer, Ph. Stee, Y. Fantei, Udo Beckmann, M. Schoeller, Karl Heinz Hofmann, C. Bailet, Michiel R. Hogerheijde, M. Lehmitz, Andreas Glindemann, Tibor Agócs, Yves Bresson, F. Allouche, Stephane Lagarde, Carsten Dominik, G. Zins, Walter Jaffe, Jean-Charles Augereau, Udo Neumann, Marco Delbo, W. Laun, P. Antonelli, Pierre Cruzalèbes, Alexis Matter, Eddy Elswijk, D. Schertl, Thomas Henning
Publikováno v:
Optical and Infrared Interferometry and Imaging VI
Optical and Infrared Interferometry and Imaging VI, Jun 2018, Austin, United States. pp.54, ⟨10.1117/12.2313388⟩
Optical and Infrared Interferometry and Imaging VI: 11-15 June 2018, Austin, Texas, United States, 1
Optical and Infrared Interferometry and Imaging VI, Jun 2018, Austin, United States. pp.54, ⟨10.1117/12.2313388⟩
Optical and Infrared Interferometry and Imaging VI: 11-15 June 2018, Austin, Texas, United States, 1
MATISSE is the second-generation mid-infrared spectrograph and imager for the Very Large Telescope Interferometer (VLTI) at Paranal. This new interferometric instrument will allow significant advances in various fundamental research fields: studying
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4717f3072932405dcc933e028a56c505
https://hal.archives-ouvertes.fr/hal-02323520
https://hal.archives-ouvertes.fr/hal-02323520