Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Cruzalèbes, Pierre"'
Autor:
Drevon, Julien, Millour, Florentin, Cruzalèbes, Pierre, Paladini, Claudia, Hron, Josef, Meilland, A., Allouche, F., Hofmann, K. -H., Lagarde, S., Lopez, B., Matter, A., Petrov, R., Robbe-Dubois, S., Schertl, D., Wittkowski, M., Zins, G., Ábrahám, P., Antonelli, P., Beckmann, U., Berio, P., Bettonvil, F., Glindemann, A., Graser, U., Heininger, M., Henning, Thomas, Isbell, Jacob W., Jaffe, Walter, Labadie, Lucas, Leinert, Christoph, Lehmitz, Michael, Morel, Sébastien, Meisenheimer, Klaus, Soulain, Anthony, Varga, Josef, Weigelt, Gerd, Woillez, Julien, Augereau, Jean-Charles, van Boekel, Roy, Burtscher, Leonard, Danchi, William, Dominik, Carsten, Gamez-Rosas, Violetta, Hocdé, Vincent, Hogerheijde, M., Klarmann, Lucia, Kokoulina, Elena, Leftley, James, Stee, Ph., Vakili, Farrokh, Waters, Rens, Wolf, Sebastian, Yoffe, Gideon
AGB stars are one of the main sources of dust production in the Galaxy. However, it is not clear what this process looks like and where the dust is condensing in the circumstellar environment. By characterizing the location of the dust and the molecu
Externí odkaz:
http://arxiv.org/abs/2208.10845
Autor:
Isbell, Jacob W., Meisenheimer, Klaus, Pott, Jörg-Uwe, Stalevski, Marko, Tristram, Konrad R. W., Sanchez-Bermudez, Joel, Hofmann, Karl-Heinz, Rosas, Violeta Gámez, Jaffe, Walter, Burtscher, Leonard, Leftley, James, Petrov, Romain, Lopez, Bruno, Henning, Thomas, Weigelt, Gerd, Allouche, Fatme, Berio, Philippe, Bettonvil, Felix, Cruzalebes, Pierre, Dominik, Carsten, Heininger, Matthias, Hogerheijde, Michiel, Lagarde, Stéphane, Lehmitz, Michael, Matter, Alexis, Millour, Florentin, Robbe-Dubois, Sylvie, Schertl, Dieter, van Boekel, Roy, Varga, Josef, Woillez, Julien
Publikováno v:
A&A 663, A35 (2022)
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:
http://arxiv.org/abs/2205.01575
Autor:
Rosas, Violeta Gamez, Isbell, Jacob W., Jaffe, Walter, Petrov, Romain G., Leftley, James H., Hofmann, Karl-Heinz, Millour, Florentin, Burtscher, Leonard, Meisenheimer, Klaus, Meilland, Anthony, Waters, Laurens B. F. M., Lopez, Bruno, Lagarde, Stephane, Weigelt, Gerd, Berio, Philippe, Allouche, Fatme, Robbe-Dubois, Sylvie, Cruzalebes, Pierre, Bettonvil, Felix, Henning, Thomas, Augereau, Jean-Charles, Antonelli, Pierre, Beckmann, Udo, van Boekel, Roy, Bendjoya, Philippe, Danchi, William C., Dominik, Carsten, Drevon, Julien, Gallimore, Jack F., Graser, Uwe, Heininger, Matthias, Hocde, Vincent, Hogerheijde, Michiel, Hron1, Josef, Impellizzeri, Caterina M. V., Klarmann, Lucia, Kokoulina, Elena, Labadie, Lucas, Lehmitz, Michael, Matter, Alexis, Paladini, Claudia, Pantin, Eric, Pott, Jorg-Uwe, Schert, Dieter, Soulain, Anthony, Stee, Philippe, Tristram, Konrad, Varga, Jozsef, Woillez, Julien, Wolf, Sebastian, Yoffe, Gideon, Zins, Gerard
In the widely accepted 'Unified Model' solution of the classification puzzle of Active Galactic Nuclei, the orientation of a dusty accretion torus around the central black hole dominates their appearance. In 'type-1' systems, the bright nucleus is vi
Externí odkaz:
http://arxiv.org/abs/2112.13694
Autor:
Boskri, Abdelkarim, Petrov, Romain G., Halkouj, Thami El, Hadjara, Massinissa, Leftley, James, Benkhaldoun, Zouhair, Cruzalèbes, Pierre, Ziad, Aziz, Carbillet, Marcel
The spectacular results provided by the second-generation VLTI instruments GRAVITY and MATISSE on active galactic nuclei (AGN) trigger and justify a strong increase in the sensitivity limit of optical interferometers. A key component of such an upgra
Externí odkaz:
http://arxiv.org/abs/2107.04729
Autor:
Stee, Philippe, Allard, France, Benisty, Myriam, Bigot, Lionel, Blind, Nicolas, Boffin, Henri, Fernandes, Marcelo Borges, Carciofi, Alex, Chiavassa, Andrea, Creevey, Orlagh, Cruzalebes, Pierre, de Wit, Willem-Jan, de Souza, Armando Domiciano, Elvis, Martin, Fabas, Nicolas, Faes, Daniel, Gallenne, Alexandre, Pena, Carlos Guerrero, Hillen, Michel, Hoenig, Sebastian, Ireland, Michael, Kervella, Pierre, Kishimoto, Makoto, Kostogryz, Nadia, Kraus, Stefan, Labeyrie, Antoine, Bouquin, Jean-Baptiste Le, Lebre, Agnès, Ligi, Roxanne, Marconi, Alessandro, Marsh, Thomas, Meilland, Anthony, Millour, Florentin, Monnier, John, Mourard, Denis, Nardetto, Nicolas, Ohnaka, Keiichi, Paladini, Claudia, Perraut, Karine, Perrin, Guy, Petit, Pascal, Petrov, Romain, Rakshit, Suvendu, Schaefer, Gail, Schneider, Jean, Shulyak, Denis, Simon, Michal, Soulez, Ferreol, Steeghs, Danny, Tallon-Bosc, Isabelle, Tallon, Michel, Brummelaar, Theo ten, Thiebaut, Eric, Thévenin, Frédéric, Van Winckel, Hans, Wittkowski, Markus, Zorec, Juan
High spatial resolution is the key for the understanding various astrophysical phenomena. But even with the future E-ELT, single dish instruments are limited to a spatial resolution of about 4 mas in the visible. For the closest objects within our Ga
Externí odkaz:
http://arxiv.org/abs/1703.02395
Autor:
Cruzalèbes, Pierre, Rabbia, Yves, Jorissen, Alain, Spang, Alain, Sacuto, Stéphane, Pasquato, Ester, Chiavassa, Andrea, Chesneau, Olivier, Fréville, Patrick
Extracting stellar fundamental parameters from SPectro-Interferometric (SPI) data requires reliable estimates of observables and with robust uncertainties (visibility, triple product, phase closure). A number of fine calibration procedures is necessa
Externí odkaz:
http://arxiv.org/abs/1304.1666
Autor:
Sacuto, Stéphane, Jorissen, Alain, Cruzalèbes, Pierre, Chesneau, Olivier, Ohnaka, Keiichi, Quirrenbach, Andreas, Lopez, Bruno
We study the close circumstellar environment of the nearby S-type star Pi^1 Gruis using high spatial-resolution, mid-infrared observations from the ESO/VLTI. Spectra and visibilities were obtained with the MIDI interferometer on the VLT Auxiliary Tel
Externí odkaz:
http://arxiv.org/abs/0803.3077
We present high spatial resolution observations of the mid-infrared core of the dusty symbiotic system HM Sge. The MIDI interferometer was used with the VLT UTs and ATs providing baselines oriented from PA=42° to 105°. The MIDI visibilities are com
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702374
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Millour, Florentin, Meilland, Anthony, Matter, Alexis, Mella, Guillaume, Bourgès, Laurent, Paladini, Claudia, Tallon-Bosc, Isabelle, Tallon, Michel, Soulez, Ferreol, Buscher, David, Mérand, Antoine, Benisty, Myriam, van Boekel, Roy, Cruzalèbes, Pierre, Defrère, Denis, Domiciano de Souza, Armando, Filho, Mercedes, Garcia, Paulo, Hönig, Sebastian, Ligi, Roxanne, Maccotta, Camille, Mckean, John, Patru, Fabien, Perraut, Karine, Pott, Jörg-Uwe, Spang, Alain, Rousset, Sophie
Publikováno v:
The Messenger, 185, 28-30
Eso Messenger
Eso Messenger, 2021, 185, pp.28-30. ⟨10.18727/0722-6691/5250⟩
Eso Messenger
Eso Messenger, 2021, 185, pp.28-30. ⟨10.18727/0722-6691/5250⟩
Very Large Telescope Inerferometer (VLTI) schools have nearly a 20-year history and have trained a significant fraction of today���s optical interferometrists who use high-angular-resolution techniques on a regular basis. Very early in the deve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a485a51a212877d1b2d30632b2a770d
https://lirias.kuleuven.be/handle/20.500.12942/693812
https://lirias.kuleuven.be/handle/20.500.12942/693812