Zobrazeno 1 - 10
of 764
pro vyhledávání: '"Schmid, V."'
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:
Schmid, V. S., Aerts, C.
Publikováno v:
A&A 592, A116 (2016)
Pulsating binary stars are ideal targets for testing the theory of stellar structure and evolution. Fundamental parameters can be derived to high precision from binary modelling and provide crucial constraints for seismic modelling. High-order gravit
Externí odkaz:
http://arxiv.org/abs/1605.07958
Autor:
Keen, M. A., Bedding, T. R., Murphy, S. J., Schmid, V. S., Aerts, C., Tkachenko, A., Ouazzani, R. -M., Kurtz, D. W.
We use four years of Kepler photometry to study the non-eclipsing spectroscopic binary KIC 10080943. We find both components to be $\gamma$ Doradus/$\delta$ Scuti hybrids, which pulsate in both p and g modes. We present an analysis of the g modes, wh
Externí odkaz:
http://arxiv.org/abs/1509.03317
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
Autor:
Buysschaert, B., Aerts, C., Bloemen, S., Debosscher, J., Neiner, C., Briquet, M., Vos, J., Papics, P., Manick, R., Schmid, V., Van Winkel, H., Tkachenko, A.
We present high-precision photometric light curves of five O-type stars observed with the refurbished {\it Kepler\/} satellite during its Campaign 0. For one of the stars, we also assembled high-resolution ground-based spectroscopy with the {\sc herm
Externí odkaz:
http://arxiv.org/abs/1507.03091
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
Akademický článek
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Autor:
Beck, P. G., Kambe, E., Hillen, M., Corsaro, E., Van Winckel, H., Moravveji, E., De Ridder, J., Bloemen, S., Saesen, S., Mathias, P., Degroote, P., Kallinger, T., Verhoelst, T., Ando, H., Carrier, F., Acke, B., Oreiro, R., Miglio, A., Eggenberger, P., Sato, B., Zwintz, K., Pápics, P. I., Marcos-Arenal, P., Fuentes, S. A. Sans, Schmid, V. S., Waelkens, C., Østensen, R., Matthews, J. M., Yoshida, M., Izumiura, H., Koyano, H., Nagayama, S., Shimizu, Y., Okada, N., Okita, K., Sakamoto, A., Yamamuro, T., Aerts, C.
Red giants are evolved stars which exhibit solar-like oscillations. Although a multitude of stars have been observed with space telescopes, only a handful of red-giant stars were targets of spectroscopic asteroseismic observing projects. We search fo
Externí odkaz:
http://arxiv.org/abs/1407.6352
Autor:
Schmid, V. S., Themeßl, N., Breger, M., Degroote, P., Aerts, C., Beck, P. G., Tkachenko, A., Van Reeth, T., Bloemen, S., Debosscher, J., Castanheira, B. G., McArthur, B. E., Pápics, P. I., Fritz, V., Falcon, R. E.
Publikováno v:
A&A 570, A33 (2014)
More than 40 years of ground-based photometric observations of the delta Sct star 4CVn revealed 18 independent oscillation frequencies, including radial as well as non-radial p-modes of low spherical degree l<=2. From 2008 to 2011, more than 2000 spe
Externí odkaz:
http://arxiv.org/abs/1407.4257
We introduce our PhD project in which we focus on pulsating stars in eclipsing binaries. The combination of high-precision Kepler photometry with high-resolution HERMES spectroscopy allows for detailed descriptions of our sample of target stars. We r
Externí odkaz:
http://arxiv.org/abs/1401.8279