Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Matthews, J. M."'
Autor:
Antoci, V., Cunha, M. S., Bowman, D. M., Murphy, S. J., Kurtz, D. W., Bedding, T. R., Borre, C. C., Christophe, S., Daszy��ska-Daszkiewicz, J., Fox-Machado, L., Hern��ndez, A. Garc��a, Ghasemi, H., Handberg, R., Hansen, H., Hasanzadeh, A., Houdek, G., Johnston, C., Justesen, A. B., Alicavus, F. Kahraman, Kotysz, K., Latham, D., Matthews, J. M., M��nster, J., Niemczura, E., Paunzen, E., Arias, J. P. S��nchez, Pigulski, A., Pepper, J., Richey-Yowell, T., Safari, H., Seager, S., Smalley, B., Shutt, T., S��dor, A., Su��rez, J. -C., Tkachenko, A., Wu, T., Zwintz, K., Forteza, S. Barcel��, Brunsden, E., Bogn��r, Z., Buzasi, D. L., Chowdhury, S., De Cat, P., Evans, J. A., Guo, Z., Guzik, J. A., Jevtic, N., Lampens, P., Martiz, M. Lares, Lovekin, C., Li, G., Mirouh, G. M., Mkrtichian, D., Monteiro, M. J. P. F. G., Nemec, J. M., Ouazzani, R., Pascual-Granado, J., Reese, D. R., Rieutord, M., Rodon, J. R., Skarka, M., Sowicka, P., Stateva, I., Szab��, R., Weiss, W. W.
We present the first asteroseismic results for $��$ Scuti and $��$ Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilise the 2-min cadence TESS data for a sample of 117 stars to classify their behaviour regarding variabili
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3b9a56b363ba0872d02caaa0ba1b6b00
Autor:
Weiss, W. W., Fr��hlich, H. -E., Pigulski, A., Popowicz, A., Huber, D., Kuschnig, R., Moffat, A. F. J., Matthews, J. M., Saio, H., Schwarzenberg-Czerny, A., Grant, C. C., Koudelka, O., L��ftinger, T., Rucinski, S. M., Wade, G. A., Alves, J., Guedel, M., Handler, G., Mochnacki, St., Orleanski, P., Pablo, B., Pamyatnykh, A., Ramiaramanantsoa, T., Rowe, J., Whittaker, G., Zawistowski, T., Zoc��onska, E., Zwintz, K.
We report on an analysis of high-precision, multi-colour photometric observations of the rapidly-oscillating Ap (roAp) star $��$ Cir. These observations were obtained with the BRITE-Constellation, which is a coordinated mission of five nanosatell
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::629ca42631a5f82edcb601f4f244f0e5
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., P��pics, P. I., Marcos-Arenal, P., Fuentes, S. A. Sans, Schmid, V. S., Waelkens, C., ��stensen, 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:
https://explore.openaire.eu/search/publication?articleId=doi_________::a0d11152d3515e6bdfcfc4a172ad0764
Autor:
Weiss, W. W., Rucinski, S. M., Moffat, A. F. J., Schwarzenberg-Czerny, A., Koudelka, O. F., Grant, C. C., Zee, R. E., Kuschnig, R., St Mochnacki, Matthews, J. M., Orleanski, P., Pamyatnykh, A., Pigulski, A., Alves, J., Manuel Guedel, Handler, G., Wade, G. A., Zwintz, K., Ccd, Team, Photometry Tiger Team
Publikováno v:
ResearcherID
BRITE-Constellation (where BRITE stands for BRIght Target Explorer) is an international nanosatellite mission to monitor photometrically, in two colours, the brightness and temperature variations of stars generally brighter than mag(V) ~ 4, with prec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0b10a414a15b3e3bb8f9821d97cc40ae
Autor:
Breger, M., Hareter, M., Endl, Markus, Kuschnig, R., Weiss, W. W., Matthews, J. M., Guenther, D. B., Moffat, A. F. J., Rowe, J. F., Rucinski, S. M., Sasselov, D.
The Praesepe cluster contains a number of Delta Sct and Gamma Dor pulsators. Asteroseismology of cluster stars is simplified by the common distance, age and stellar abundances. Since asteroseismology requires a large number of known frequencies, the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aaa9d4d09428daef63e2d82a9f67e086
Autor:
Casey, M. P., Zwintz, K., Guenther, D. B., Weiss, W. W., Amado, P. J., D��az-Fraile, D., Rodriguez, E., Kuschnig, R., Matthews, J. M., Moffat, A. F. J., Rowe, J. F., Rucinski, S. M., Sasselov, D.
MOST observations and model analysis of the Herbig Ae star HD 34282 (V1366 Ori) reveal ��-Scuti pulsations. 22 frequencies are observed, 10 of which confirm those previously identified by Amado et al. (2006), and 12 of which are newly discovered
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::864d06358dd8f87b89a1a22b470307f0
Autor:
Grunhut, J. H., Rivinius, Th., Wade, G. A., Townsend, R. H. D., Marcolino, W. L. F., Bohlender, D. A., Szeifert, Th., Petit, V., Matthews, J. M., Rowe, J. F., Moffat, A. F. J., Kallinger, T., Kuschnig, R., Guenther, B. D., Rucinski, S. M., Sasselov, D., Weiss, W. W., Collaboration, the MiMeS
We report the discovery and analysis of a very strong magnetic field in the rapidly rotating early B-type star HR 5907, based on observations obtained as part of the Magnetism in Massive Stars (MiMeS) project. We infer a rotation period of 0.508276 +
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55d5491091b66c6a7be2204eee1a27d8
Precise time-series photometry with the MOST satellite has led to identification of 10 pulsation frequencies in the rapidly oscillating Ap (roAp) star HD 134214. We have fitted the observed frequencies with theoretical frequencies of axisymmetric mod
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f54bbf752805541b2c3fb29928f75c2a
Autor:
Cameron, C., Saio, H., Kuschnig, R., Walker, G. A. H., Matthews, J. M., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M., Sasselov, D., Weiss, W. W.
The MOST (Microvariability and Oscillations of Stars) satellite has discovered SPBe (Slowly Pulsating Be) oscillations in the stars HD 127756 (B1/B2 Vne) and HD 217543 (B3 Vpe). For HD 127756, 30 significant frequencies are identified from 31 days of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2a4b076aebab5ba577c09c557726f16e
Autor:
Gruberbauer, M., Saio, H., Huber, D., Kallinger, T., Weiss, W. W., Guenther, D. B., Kuschnig, R., Matthews, J. M., Moffat, A. F. J., Rucinski, S., Sasselov, D., Walker, G. A. H.
Aims. Despite photometry and spectroscopy of its oscillations obtained over the past 25 years, the pulsation frequency spectrum of the rapidly oscillating Ap (roAp) star gamma Equ has remained poorly understood. Better time-series photometry, combine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10010c9f094e7b4ed004da6d6dfeb685