Zobrazeno 1 - 10
of 112
pro vyhledávání: '"Bloecker, T."'
Autor:
Millour, F., Petrov, R. G., Chesneau, O., Bonneau, D., Dessart, L., Bechet, C., Tallon-Bosc, I., Tallon, M., Thiébaut, E., Vakili, F., Malbet, F., Mourard, D., Zins, G., Roussel, A., Robbe-Dubois, S., Puget, P., Perraut, K., Lisi, F., Coarer, E. Le, Lagarde, S., Kern, P., Glück, L., Duvert, G., Chelli, A., Bresson, Y., Beckmann, U., Antonelli, P., Weigelt, G., Ventura, N., Vannier, M., Valtier, J. -C., Testi, L., Tatulli, E., Tasso, D., Stefanini, P., Stee, P., Solscheid, W., Schertl, D., Salinari, P., Sacchettini, M., Richichi, A., Reynaud, F., Rebattu, S., Rabbia, Y., Preibisch, T., Perrier, C., Pacini, F., Ohnaka, K., Nussbaum, E., Mouillet, D., Monin, J. -L., Mège, P., Mathias, P., Martinot-Lagarde, G., Mars, G., Marconi, A., Magnard, Y., Lopez, B., Contel, D. Le, Contel, J. -M. Le, Kraus, S., Kamm, D., Hofmann, K. -H., Utrera, O. Hernandez, Heininger, M., Heiden, M., Gil, C., Giani, E., Glentzlin, A., Gennari, S., Gallardo, A., Fraix-Burnet, D., Foy, R., Fossat, E., Forveille, T., Ferruzzi, D., Feautrier, P., Dugué, M., Driebe, T., De Souza, A. Domiciano, Delboulbé, A., Connot, C., Colin, J., Clausse, J. -M., Cassaing, F., Busoni, S., Bonhomme, S., Blöcker, T., Behrend, J., Baffa, C., Aristidi, E., Arezki, B., Agabi, K., Acke, B., Accardo, M., Kiekebusch, M., Rantakyrö, F., Schoeller, Markus
In this work, we present the first AMBER observations, of the Wolf-Rayet and O (WR+O) star binary system y2 Velorum. The AMBER instrument was used with the telescopes UT2, UT3, and UT4 on baselines ranging from 46m to 85m. It delivered spectrally dis
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610936
Autor:
Bloecker, T.
The structure and evolution of central stars of planetary nebulae (CSPNe) is reviewed. CSPNe represent the rapid transitional stage between the Asymptotic Giant Branch (AGB) and the white-dwarf domain. It is shown that the whole evolution off the AGB
Externí odkaz:
http://arxiv.org/abs/astro-ph/0207161
Interferometric observations of stars in late stages of stellar evolution and the impact of VLTI observations are discussed. Special attention is paid to the spectral information that can be derived from these observations and on the corresponding as
Externí odkaz:
http://arxiv.org/abs/astro-ph/0207093
Autor:
Hofmann, K. -H., Beckmann, U., Bloecker, T., Foresto, V. Coude du, Lacasse, M., Mennesson, B., Millan-Gabet, R., Morel, S., Perrin, G., Pras, B., Ruilier, C., Schertl, D., Schoeller, M., Scholz, M., Shenavrin, V., Traub, W., Weigelt, G., Wittkowski, M., Yudin, B.
Publikováno v:
New Astron. 7 (2002) 9
We present K'-band observations of five Mira stars with the IOTA interferometer. The interferograms were obtained with the FLUOR fiber optics beam combiner, which provides high-accuracy visibility measurements in spite of time-variable atmospheric co
Externí odkaz:
http://arxiv.org/abs/astro-ph/0206406
We present new near-infrared (JHK) bispectrum speckle-interferometry monitoring of the carbon star IRC+10216 obtained between 1999 and 2001 with the SAO 6m telescope. The J-, H-, and K-band resolutions are 50mas, 56mas, and 73mas, resp. The total seq
Externí odkaz:
http://arxiv.org/abs/astro-ph/0206309
Autor:
Ohnaka, K., Balega, Y., Bloecker, T., Efimov, Y. S., Hofmann, K. -H., Ikhsanov, N. R., Shenavrin, V. I., Weigelt, G., Yudin, B. F.
Publikováno v:
Astronomy & Astrophysics 380, 212-220 (2001)
We present the first speckle interferometric observations of R CrB, the prototype of a class of peculiar stars which undergo irregular declines in their visible light curves. The observations were carried out with the 6m telescope at the Special Astr
Externí odkaz:
http://arxiv.org/abs/astro-ph/0201049
WR 118 is a highly evolved Wolf-Rayet star of the WC10 subtype surrounded by a permanent dust shell absorbing and re-emitting in the infrared a considerable fraction of the stellar luminosity. We present the first diffraction-limited 2.13micron speck
Externí odkaz:
http://arxiv.org/abs/astro-ph/0110132
(abridged) CIT 3 is an oxygen-rich long-period variable evolving along the AGB and one of the most extreme infrared AGB objects. We present the first bispectrum speckle-interferometry observations of CIT 3 in the J-, H-, and K'-band (resolution: 48ma
Externí odkaz:
http://arxiv.org/abs/astro-ph/0110108
Structural and chemical changes during the AGB and post-AGB evolution are discussed with respect to two recent observational and theoretical findings. On the one hand, high-resolution infrared observations revealed details of the dynamical evolution
Externí odkaz:
http://arxiv.org/abs/astro-ph/0102383
Autor:
Bloecker, T.
Publikováno v:
Astrophys.Space Sci. 275 (2001) 1-14
The evolution on the AGB and beyond is reviewed with respect to the origin of Wolf-Rayet central stars. We focus on thermal pulses due to their particular importance for the evolution of hydrogen deficient stars. It is shown that overshoot applied to
Externí odkaz:
http://arxiv.org/abs/astro-ph/0102135