Zobrazeno 1 - 10
of 221
pro vyhledávání: '"Smedt, K."'
Autor:
Royer, P., Merle, T., Dsilva, K., Sekaran, S., Van Winckel, H., Frémat, Y., Van der Swaelmen, M., Gebruers, S., Tkachenko, A., Laverick, M., Dirickx, M., Raskin, G., Hensberge, H., Abdul-Masih, M., Acke, B., Alonso, M. L., Mahato, S. Bandhu, Beck, P. G., Behara, N., Bloemen, S., Buysschaert, B., Cox, N., Debosscher, J., De Cat, P., Degroote, P., De Nutte, R., De Smedt, K., de Vries, B., Dumortier, L., Escorza, A., Exter, K., Goriely, S., Gorlova, N., Hillen, M., Homan, W., Jorissen, A., Kamath, D., Karjalainen, M., Karjalainen, R., Lampens, P., Lobel, A., Lombaert, R., Marcos-Arenal, P., Menu, J., Merges, F., Moravveji, E., Nemeth, P., Neyskens, P., Ostensen, R., Pápics, P. I., Perez, J., Royer, S. Prins S., Samadi-Ghadim, A., Sana, H., Fuentes, A. Sans, Scaringi, S., Schmid, V., Siess, L., Siopis, C., Smolders, K., Sodor, S., Thoul, A., Triana, S., Vandenbussche, B., Van de Sande, M., Van De Steene, G., Van Eck, S., van Hoof, P. A. M., Van Marle, A. J., Van Reeth, T., Vermeylen, L., Volpi, D., Vos, J., Waelkens, C.
Publikováno v:
A&A 681, A107 (2024)
Over the past decades, libraries of stellar spectra have been used in a large variety of science cases, including as sources of reference spectra for a given object or a given spectral type. Despite the existence of large libraries and the increasing
Externí odkaz:
http://arxiv.org/abs/2311.02705
Autor:
Pápics, P. I., Tkachenko, A., Van Reeth, T., Aerts, C., Moravveji, E., Van de Sande, M., De Smedt, K., Bloemen, S., Southworth, J., Debosscher, J., Niemczura, E., Gameiro, J. F.
Publikováno v:
A&A 598, A74 (2017)
Massive stars are important building blocks of the Universe, and their stellar structure and evolution models are fundamental cornerstones of various fields in modern astrophysics. The precision of these models is limited by our lack of understanding
Externí odkaz:
http://arxiv.org/abs/1611.06955
Autor:
Di Mauro, M . P., Ventura, R., Cardini, D., Stello, D., Christensen-Dalsgaard, J., Dziembowski, W. A., Paterno', L., Beck, P. G., Bloemen, S., Davies, G. R., De Smedt, K., Elsworth, Y., Garcia, R. A., Hekker, S., Mosser, B., Tkachenko, A.
In this paper we study the dynamics of the stellar interior of the early red-giant star KIC 4448777 by asteroseismic inversion of 14 splittings of the dipole mixed modes obtained from {\it Kepler} observations. In order to overcome the complexity of
Externí odkaz:
http://arxiv.org/abs/1511.06160
Publikováno v:
A&A 583, A77 (2015)
We explore modifications to the current scenario for the slow neutron capture process in asymptotic giant branch (AGB) stars to account for the Pb deficiency observed in post-AGB stars of low metallicity ([Fe/H] ~ -1.2) and low initial mass (~ 1 - 1.
Externí odkaz:
http://arxiv.org/abs/1509.03518
Autor:
Schmid, V. S., Tkachenko, A., Aerts, C., Degroote, P., Bloemen, S., Murphy, S. J., Van Reeth, T., Papics, P. I., Bedding, T. R., Keen, M. A., Prsa, A., Menu, J., Debosscher, J., Hrudkova, M., De Smedt, K., Lombaert, R., Nemeth, P.
Publikováno v:
A&A 584, A35 (2015)
Gamma Doradus and delta Scuti pulsators cover the transition region between low mass and massive main-sequence stars, and as such, are critical for testing stellar models. When they reside in binary systems, we can combine two independent methods to
Externí odkaz:
http://arxiv.org/abs/1509.00781
Context: This paper is part of a larger project in which we study the chemical abundances of extra-galactic post-AGB stars with the ultimate goal of improving our knowledge of the poorly understood AGB third dredge-up mixing processes and s-process n
Externí odkaz:
http://arxiv.org/abs/1508.01091
We present a detailed study based on infrared photometry of all Galactic RV Tauri stars from the General Catalogue of Variable Stars (GCVS). RV Tauri stars are the brightest among the population II Cepheids. They are thought to evolve away from the a
Externí odkaz:
http://arxiv.org/abs/1507.04175
Autor:
Van Reeth, T., Tkachenko, A., Aerts, C., Papics, P. I., Triana, S. A., Zwintz, K., Degroote, P., Debosscher, J., Bloemen, S., Schmid, V. S., De Smedt, K., Fremat, Y., Fuentes, A. S., Homan, W., Hrudkova, M., Karjalainen, R., Lombaert, R., Nemeth, P., Oestensen, R., Van De Steene, G., Vos, J., Raskin, G., Van Winckel, H.
Gamma Doradus stars (hereafter gamma Dor stars) are gravity-mode pulsators of spectral type A or F. Such modes probe the deep stellar interior, offering a detailed fingerprint of their structure. Four-year high-precision space-based Kepler photometry
Externí odkaz:
http://arxiv.org/abs/1504.02119
Autor:
Pápics, P. I., Tkachenko, A., Aerts, C., Van Reeth, T., De Smedt, K., Hillen, M., Oestensen, R., Moravveji, E.
We present the first detection of a rotationally affected series consisting of 36 consecutive high-order sectoral dipole gravity modes in a slowly pulsating B (SPB) star. The results are based on the analysis of four years of virtually uninterrupted
Externí odkaz:
http://arxiv.org/abs/1504.00496
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