Zobrazeno 1 - 10
of 2 949
pro vyhledávání: '"Morris, R. L."'
Autor:
DESILVA, JENNIFER MARA
Publikováno v:
Renaissance and Reformation / Renaissance et Réforme, 2019 Apr 01. 42(2), 237-240.
Externí odkaz:
https://www.jstor.org/stable/26860694
Autor:
Close, Christopher W.1
Publikováno v:
Sixteenth Century Journal. Summer2022, Vol. 53 Issue 2, p488-490. 3p.
Akademický článek
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Autor:
Mosser, B., Goupil, M. J., Belkacem, K., Marques, J. P., Beck, P. G., Bloemen, S., De Ridder, J., Barban, C., Deheuvels, S., Elsworth, Y., Hekker, S., Kallinger, T., Ouazzani, R. M., Pinsonneault, M., Samadi, R., Stello, D., Garcia, R. A., Klaus, T. C., Li, J., Mathur, S., Morris, R. L.
The space mission Kepler provides us with long and uninterrupted photometric time series of red giants. We are now able to probe the rotational behaviour in their deep interiors using the observations of mixed modes. We aim to measure the rotational
Externí odkaz:
http://arxiv.org/abs/1209.3336
Autor:
Silvotti, R., Østensen, R. H., Bloemen, S., Telting, J. H., Heber, U., Oreiro, R., Reed, M. D., Farris, L. E., O'Toole, S. J., Lanteri, L., Degroote, P., Hu, H., Baran, A. S., Hermes, J. J., Althaus, L. G., Marsh, T. R., Charpinet, S., Li, J., Morris, R. L., Sanderfer, D. T.
We have used 605 days of photometric data from the Kepler spacecraft to study KIC 6614501, a close binary system with an orbital period of 0.15749747(25) days (3.779939 hours), that consists of a low-mass subdwarf B (sdB) star and a white dwarf. As s
Externí odkaz:
http://arxiv.org/abs/1205.2457
Autor:
Tkachenko, A., Aerts, C., Pavlovski, K., Southworth, J., Degroote, P., Debosscher, J., Still, M., Bryson, S., Molenberghs, G., Bloemen, S., de Vries, B. L., Hrudkova, M., Lombaert, R., Neyskens, P., Papics, P. I., Raskin, G., Van Winckel, H., Morris, R. L., Sanderfer, D. T., Seader, S. E.
We report the discovery of low-amplitude gravity-mode oscillations in the massive binary star V380 Cyg, from 180 d of Kepler custom-aperture space photometry and 5 months of high-resolution high signal-to-noise spectroscopy. The new data are of unpre
Externí odkaz:
http://arxiv.org/abs/1205.0554
Autor:
Bruntt, H., Basu, S., Smalley, B., Chaplin, W. J., Verner, G. A., Bedding, T. R., Catala, C., Gazzano, J. -C., Molenda-Zakowicz, J., Thygesen, A. O., Uytterhoeven, K., Hekker, S., Huber, D., Karoff, C., Mathur, S., Mosser, B., Appourchaux, T., Campante, T. L., Elsworth, Y., Garcia, R. A., Handberg, R., Metcalfe, T. S., Quirion, P. -O., Regulo, C., Roxburgh, I. W., Stello, D., Christensen-Dalsgaard, J., Kawaler, S. D., Kjeldsen, H., Morris, R. L., Quintana, E. V., Sanderfer, D. T.
We present a detailed spectroscopic study of 93 solar-type stars that are targets of the NASA/Kepler mission and provide detailed chemical composition of each target. We find that the overall metallicity is well-represented by Fe lines. Relative abun
Externí odkaz:
http://arxiv.org/abs/1203.0611
Autor:
Mosser, B., Elsworth, Y., Hekker, S., Huber, D., Kallinger, T., Mathur, S., Belkacem, K., Goupil, M. J., Samadi, R., Barban, C., Bedding, T. R., Chaplin, W. J., Garcia, R. A., Stello, D., De Ridder, J., Middour, C. K., Morris, R. L., Quintana, E. V
We aim to describe the oscillation power excess observed in Kepler red giants, and to investigate empirical scaling relations governing these parameters. From these scalings relations, we derive new physical properties of red giant oscillations. Vari
Externí odkaz:
http://arxiv.org/abs/1110.0980
Publikováno v:
MNRAS, 414, 2950 (2011)
The amplitude and phase modulation observed in a significant fraction of the RR Lyrae variables - the Blazhko effect - represents a long-standing enigma in stellar pulsation theory. No satisfactory explanation for the Blazhko effect has been proposed
Externí odkaz:
http://arxiv.org/abs/1102.4845