Zobrazeno 21 - 30
of 155
pro vyhledávání: '"van Boekel, Roy"'
Autor:
Sanchez-Bermudez, Joel, Millour, Florentin, Baron, Fabien, van Boekel, Roy, Bourgès, Laurent, Duvert, Gilles, Garcia, Paulo J. V., Gomes, Nuno, Hofmann, Karl-Heinz, Henning, Thomas, Isbell, Jacob W., Lopez, Bruno, Matter, Alexis, Pott, J-Uwe, Schertl, Dieter, Thiébaut, Eric, Weigelt, Gerd, Young, John
During the last two decades, the first generation of beam combiners at the Very Large Telescope Interferometer has proved the importance of optical interferometry for high-angular resolution astrophysical studies in the near- and mid-infrared. With t
Externí odkaz:
http://arxiv.org/abs/1812.06191
Autor:
Jamialahmadi, Narges, Ratzka, Thorsten, Panic, Olja, Fathivavsari, Hassan, Van Boekel, Roy, Flement, Sebastien, Hening, Thomas, Jaffe, Walter, Mulders, Gijs
We refine the gap size measurements of the disk surrounding the Herbig Ae star HD 100546 in the N band. Our new mid-infrared interferometric (MIDI) data have been taken with the UT baselines and span the full range of orientations. The correlated flu
Externí odkaz:
http://arxiv.org/abs/1808.05052
Autor:
Bean, Jacob L., Stevenson, Kevin B., Batalha, Natalie M., Berta-Thompson, Zachory, Kreidberg, Laura, Crouzet, Nicolas, Benneke, Björn, Line, Michael R., Sing, David K., Wakeford, Hannah R., Knutson, Heather A., Kempton, Eliza M. -R., Désert, Jean-Michel, Crossfield, Ian, Batalha, Natasha E., de Wit, Julien, Parmentier, Vivien, Harrington, Joseph, Moses, Julianne I., Lopez-Morales, Mercedes, Alam, Munazza K., Blecic, Jasmina, Bruno, Giovanni, Carter, Aarynn L., Chapman, John W., Decin, Leen, Dragomir, Diana, Evans, Thomas M., Fortney, Jonathan J., Fraine, Jonathan D., Gao, Peter, Muñoz, Antonio García, Gibson, Neale P., Goyal, Jayesh M., Heng, Kevin, Hu, Renyu, Kendrew, Sarah, Kilpatrick, Brian M., Krick, Jessica, Lagage, Pierre-Olivier, Lendl, Monika, Louden, Tom, Madhusudhan, Nikku, Mandell, Avi M., Mansfield, Megan, May, Erin M., Morello, Giuseppe, Morley, Caroline V., Nikolov, Nikolay, Redfield, Seth, Roberts, Jessica E., Schlawin, Everett, Spake, Jessica J., Todorov, Kamen O., Tsiaras, Angelos, Venot, Olivia, Waalkes, William C., Wheatley, Peter J., Zellem, Robert T., Angerhausen, Daniel, Barrado, David, Carone, Ludmila, Casewell, Sarah L., Cubillos, Patricio E., Damiano, Mario, de Val-Borro, Miguel, Drummond, Benjamin, Edwards, Billy, Endl, Michael, Espinoza, Nestor, France, Kevin, Gizis, John E., Greene, Thomas P., Henning, Thomas K., Hong, Yucian, Ingalls, James G., Iro, Nicolas, Irwin, Patrick G. J., Kataria, Tiffany, Lahuis, Fred, Leconte, Jérémy, Lillo-Box, Jorge, Lines, Stefan, Lothringer, Joshua D., Mancini, Luigi, Marchis, Franck, Mayne, Nathan, Palle, Enric, Rauscher, Emily, Roudier, Gaël, Shkolnik, Evgenya L., Southworth, John, Swain, Mark R., Taylor, Jake, Teske, Johanna, Tinetti, Giovanna, Tremblin, Pascal, Tucker, Gregory S., van Boekel, Roy, Waldmann, Ingo P., Weaver, Ian C., Zingales, Tiziano
The James Webb Space Telescope (JWST) presents the opportunity to transform our understanding of planets and the origins of life by revealing the atmospheric compositions, structures, and dynamics of transiting exoplanets in unprecedented detail. How
Externí odkaz:
http://arxiv.org/abs/1803.04985
Autor:
Garufi, Antonio, Benisty, Myriam, Stolker, Tomas, Avenhaus, Henning, de Boer, Jos, Pohl, Adriana, Quanz, Sascha P., Dominik, Carsten, Ginski, Christian, Thalmann, Christian, van Boekel, Roy, Boccaletti, Anthony, Henning, Thomas, consortium, SPHERE
Spatially resolving the immediate surroundings of young stars is a key challenge for the planet formation community. SPHERE on the VLT represents an important step forward by increasing the opportunities offered by optical or near-infrared imaging in
Externí odkaz:
http://arxiv.org/abs/1710.02795
Autor:
Liu, Yao, Henning, Thomas, Carrasco-Gonzalez, Carlos, Chandler, Claire J., Linz, Hendrik, Birnstiel, Til, van Boekel, Roy, Perez, Laura M., Flock, Mario, Testi, Leonardo, Rodriguez, Luis F., Galvan-Madrid, Roberto
Publikováno v:
A&A 607, A74 (2017)
We conducted a detailed radiative transfer modeling of the dust emission from the circumstellar disk around HL Tau. The goal of our study is to derive the surface density profile of the inner disk and its structure. In addition to the Atacama Large M
Externí odkaz:
http://arxiv.org/abs/1708.03238
Autor:
Garufi, Antonio, Meeus, Gwendolyn, Benisty, Myriam, Quanz, Sascha, Banzatti, Andrea, Kama, Mihkel, Canovas, Hector, Eiroa, Carlos, Schmid, Hans Martin, Stolker, Tomas, Pohl, Adriana, Rigliaco, Elisabetta, Menard, Francois, Meyer, Micheal, van Boekel, Roy, Dominik, Carsten
Publikováno v:
A&A 603, A21 (2017)
High-resolution imaging reveals a large morphological variety of protoplanetary disks. To date, no constraints on their global evolution have been found from this census. An evolutionary classification of disks was proposed based on their IR spectral
Externí odkaz:
http://arxiv.org/abs/1703.01512
Autor:
Mollière, Paul, van Boekel, Roy, Bouwman, Jeroen, Henning, Thomas, Lagage, Pierre-Olivier, Min, Michiel
Publikováno v:
A&A 600, A10 (2017)
The James Webb Space Telescope will enable astronomers to obtain exoplanet spectra of unprecedented precision. Especially the MIRI instrument may shed light on the nature of the cloud particles obscuring planetary transmission spectra in the optical
Externí odkaz:
http://arxiv.org/abs/1611.08608
Autor:
van Boekel, Roy, Henning, Thomas, Menu, Jonathan, de Boer, Jos, Langlois, Maud, Müller, André, Avenhaus, Henning, Boccaletti, Anthony, Schmid, Hans Martin, Thalmann, Christian, Benisty, Myriam, Dominik, Carsten, Ginski, Christian, Girard, Julien H., Gisler, Daniel, Gomes, Aiara Lobo, Menard, Francois, Min, Michiel, Pavlov, Alexey, Pohl, Adriana, Quanz, Sascha P., Rabou, Patrick, Roelfsema, Ronald, Sauvage, Jean-François, Teague, Rich, Wildi, Francois, Zurlo, Alice
We present scattered light images of the TW Hya disk performed with SPHERE in PDI mode at 0.63, 0.79, 1.24 and 1.62 micron. We also present H2/H3-band ADI observations. Three distinct radial depressions in the polarized intensity distribution are see
Externí odkaz:
http://arxiv.org/abs/1610.08939
The composition of a planet's atmosphere is determined by its formation, evolution, and present-day insolation. A planet's spectrum therefore may hold clues on its origins. We present a "chain" of models, linking the formation of a planet to its obse
Externí odkaz:
http://arxiv.org/abs/1609.03019
Autor:
Carrasco-Gonzalez, Carlos, Henning, Thomas, Chandler, Claire J., Linz, Hendrik, Perez, Laura, Rodriguez, Luis F., Galvan-Madrid, Roberto, Anglada, Guillem, Birnstiel, Til, van Boekel, Roy, Flock, Mario, Klahr, Hubert, Macias, Enrique, Menten, Karl, Osorio, Mayra, Testi, Leonardo, Torrelles, Jose M., Zhu, Zhaohuan
The first long-baseline ALMA campaign resolved the disk around the young star HL Tau into a number of axisymmetric bright and dark rings. Despite the very young age of HL Tau these structures have been interpreted as signatures for the presence of (p
Externí odkaz:
http://arxiv.org/abs/1603.03731