Zobrazeno 1 - 10
of 573
pro vyhledávání: '"Briquet M."'
Autor:
Aerts, C., Pedersen, M. G., Vermeyen, E., Hendriks, L., Johnston, C., Tkachenko, A., Pápics, P. I., Debosscher, J., Briquet, M., Thoul, A., Rainer, M., Poretti, E.
Publikováno v:
A&A 624, A75 (2019)
Space asteroseismology reveals that stellar structure and evolution models of intermediate- and high-mass stars are in need of improvement in terms of angular momentum and chemical element transport. We aim to probe the interior structure of a hot ma
Externí odkaz:
http://arxiv.org/abs/1902.04093
Publikováno v:
A&A 605, A104 (2017)
Large-scale magnetic fields at the surface of massive stars do not only influence the outer-most layers of the star, but also have consequences for the deep interior, only observationally accessible through asteroseismology. We performed a detailed c
Externí odkaz:
http://arxiv.org/abs/1707.09148
Autor:
Hubrig, S., Przybilla, N., Korhonen, H., Ilyin, I., Schöller, M., Jarvinen, S. P., Nieva, M. -F., Scholz, R. -D., Kimeswenger, S., Ramolla, M., Kholtygin, A. F., Briquet, M.
The magnetic field of CPD -57 3509 was recently detected in the framework of the BOB (B fields in OB stars) collaboration. We acquired low-resolution spectropolarimetric observations of CPD -57 3509 with FORS2 and high-resolution UVES observations ra
Externí odkaz:
http://arxiv.org/abs/1707.09017
Autor:
Andrade, L., Janot-Pacheco, E., Emilio, M., Frémat, Y., Neiner, C., Poretti, E., Mathias, P., Rainer, M., Suárez, J. C., Uytterhoeven, K., Briquet, M., Diago, P. D., Fabregat, J., Gutiérrez-Soto, J.
Publikováno v:
A&A 603, A41 (2017)
We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characteristics. Classical Be stars are main-sequence objects of mainly B-type
Externí odkaz:
http://arxiv.org/abs/1705.06971
Autor:
Schoeller, M., Hubrig, S., Fossati, L., Carroll, T. A., Briquet, M., Oskinova, L. M., Jarvinen, S., Ilyin, I., Castro, N., Morel, T., Langer, N., Przybilla, N., Nieva, M. F., Kholtygin, A. F., Sana, H., Herrero, A., Barba, R. H., de Koter, A., collaboration, the BOB
Publikováno v:
A&A 599, A66 (2017)
The "B fields in OB stars" (BOB) collaboration is based on an ESO Large Programme, to study the occurrence rate, properties, and ultimately the origin of magnetic fields in massive stars. In the framework of this programme, we carried out low-resolut
Externí odkaz:
http://arxiv.org/abs/1611.04502
Among the early B-type stars, He-rich Bp stars exhibit the strongest large-scale organized magnetic fields with a predominant dipole contribution. The presence of $\beta$ Cep-like pulsations in the typical magnetic early Bp-type star HD 96446 was ann
Externí odkaz:
http://arxiv.org/abs/1610.03629
Autor:
Guzik, J. A., Houdek, G., Chaplin, W. J., Smalley, B., Kurtz, D. W., Gilliland, R. L., Mullally, F., Rowe, J. F., Bryson, S. T., Still, M. D., Antoci, V., Appourchaux, T., Basu, S., Bedding, T. R., Benomar, O., Garcia, R. A., Huber, D., Kjeldsen, H., Latham, D. W., Metcalfe, T. S., Pápics, P. I., White, T. R., Aerts, C., Ballot, J., Boyajian, T. S., Briquet, M., Bruntt, H., Buchhave, L. A., Campante, T. L., Catanzaro, G., Christensen-Dalsgaard, J., Davies, G. R., Doğan, G., Dragomir, D., Doyle, A. P., Elsworth, Y., Frasca, A., Gaulme, P., Gruberbauer, M., Handberg, R., Hekker, S., Karoff, C., Lehmann, H., Mathias, P., Mathur, S., Miglio, A., Molenda-Żakowicz, J., Mosser, B., Murphy, S. J., Régulo, C., Ripepi, V., Salabert, D., Sousa, S. G., Stello, D., Uytterhoeven, K.
$\theta$ Cygni is an F3 spectral-type main-sequence star with visual magnitude V=4.48. This star was the brightest star observed by the original Kepler spacecraft mission. Short-cadence (58.8 s) photometric data using a custom aperture were obtained
Externí odkaz:
http://arxiv.org/abs/1607.01035
Publikováno v:
A&A 587, A126 (2016)
Aims. The main-sequence B-type star $\zeta$ Cassiopeiae is known as a N-rich star with a magnetic field discovered with the Musicos spectropolarimeter. We model the magnetic field of the star by means of 82 new spectropolarimetric observations of hig
Externí odkaz:
http://arxiv.org/abs/1601.04517
Autor:
Wade, G. A., Neiner, C., Alecian, E., Grunhut, J. H., Petit, V., de Batz, B., Bohlender, D. A., Cohen, D. H., Henrichs, H. F., Kochukhov, O., Landstreet, J. D., Manset, N., Martins, F., Mathis, S., Oksala, M. E., Owocki, S. P., Rivinius, Th., Shultz, M. E., Sundqvist, J. O., Townsend, R. H. D., ud-Doula, A., Bouret, J. -C., Braithwaite, J., Briquet, M., Carciofi, A. C., David-Uraz, A., Folsom, C. P., Fullerton, A. W., Leroy, B., Marcolino, W. L. F., Moffat, A. F. J., Nazé, Y., Aurière, M., Bagnulo, S., Bailey, J. D., Barbá, R. H., Blazère, A., Böhm, T., Catala, C., Donati, J. -F., Ferrario, L., Harrington, D., Howarth, I. D., Ignace, R., Kaper, L., Lüftinger, T., Prinja, R., Vink, J. S., Weiss, W. W., Yakunin, I.
Publikováno v:
MNRAS, 456, 2-22 (2016)
The MiMeS project is a large-scale, high resolution, sensitive spectropolarimetric investigation of the magnetic properties of O and early B type stars. Initiated in 2008 and completed in 2013, the project was supported by 3 Large Program allocations
Externí odkaz:
http://arxiv.org/abs/1511.08425
Autor:
De Cat, P., Fu, J. N., Ren, A. B., Yang, X. H., Shi, J. R., Luo, A. L., Yang, M., Wang, J. L., Zhang, H. T., Shi, H. M., Zhang, W., Dong, Subo, Catanzaro, G., Corbally, C. J., Frasca, A., Gray, R. O., Molenda-Zakowicz, J., Uytterhoeven, K., Briquet, M., Bruntt, H., Frandsen, S., Kiss, L., Kurtz, D. W., Marconi, M., Niemczura, E., Oestensen, R. H., Ripepi, V., Smalley, B., Southworth, J., Szabo, R., Telting, J. H., Karoff, C., Aguirre, V. Silva, Wu, Y., Hou, Y. H., Jin, G., Zhou, X. L.
The nearly continuous light curves with micromagnitude precision provided by the space mission Kepler are revolutionising our view of pulsating stars. They have revealed a vast sea of low-amplitude pulsation modes that were undetectable from Earth. T
Externí odkaz:
http://arxiv.org/abs/1508.06391