Zobrazeno 1 - 10
of 262
pro vyhledávání: '"K Uytterhoeven"'
Autor:
K. R. Pollard, P. M. Kilmartin, Z. Kołaczkowski, Esin Soydugan, K. Uytterhoeven, J. H. Telting, E. Niemczura, Jakub Ostrowski, Ennio Poretti, Monica Rainer, F. Kahraman Aliçavuş, P. De Cat, L. Mantegazza, Juan Carlos Suárez
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 458:2307-2322
We present a spectroscopic survey of known and candidate $\gamma$\,Doradus stars. The high-resolution, high signal-to-noise spectra of 52 objects were collected by five different spectrographs. The spectral classification, atmospheric parameters (\te
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c9576d1e831c903493a7c9a5d689c302
https://doi.org/10.1093/mnras/stw393
https://doi.org/10.1093/mnras/stw393
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 447:2970-2980
Hybrid stars of the gamma Doradus and delta Scuti pulsation types have great potential for asteroseismic analysis to explore their interior structure. To achieve this, mode identifications of pulsational frequencies observed in the stars must be made
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d508bc9caf0e684ae3ecb295bc36fe7a
https://doi.org/10.1093/mnras/stu2615
https://doi.org/10.1093/mnras/stu2615
Autor:
Joanna Molenda-Zakowicz, K. Uytterhoeven, Joyce A. Guzik, Karen Kinemuchi, Jason Jackiewicz, Paul A. Bradley
Publikováno v:
Astronomical Review. 11:1-24
The high precision long time-series photometry of the NASA Kepler spacecraft provides an excellent means to discover and characterize variability in main-sequence stars, and to make progress in interpreting the pulsations to derive stellar interior s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::754000c9cff7142ddf664030e9043bbd
https://doi.org/10.1080/21672857.2015.1023120
https://doi.org/10.1080/21672857.2015.1023120
Autor:
Saskia Hekker, Laurent Eyer, K. R. Pollard, Márcio Catelan, Dennis Stello, K. Uytterhoeven, David Mkrtichian, C. Simon Jeffery, Katrien Kolenberg, Gerald Handler, Souza Oliveira Kepler, Klaus G. Strassmeier
Publikováno v:
Proceedings of the International Astronomical Union
The study of variable stars has played a central role in astronomy for over 400 years, and more so in the present than at any time in history. Stars, especially variable stars, are astrophysical laboratories for understanding physical processes in th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b3f7aaf62477aa2f7d598b01236db08
Autor:
A. Triviño Hage, G. Michalska, Jens Jessen-Hansen, E. Niemczura, Magdalena Polińska, Z. Kołaczkowski, J. Lykke, Simon J. Murphy, K. Uytterhoeven, Barry Smalley
Publikováno v:
Niemczura, E, Polinska, M, Murphy, S J, Smalley, B, Kolaczkowski, Z, Jessen-Hansen, J, Uytterhoeven, K, Lykke, J M, Trivino Hage, A & Michalska, G 2017, ' Spectroscopic survey of Kepler stars-II. FIES/NOT observations of A-and F-type stars ', Royal Astronomical Society. Monthly Notices, vol. 470, no. 3, pp. 2870-2889 . https://doi.org/10.1093/mnras/stx1256
We have analysed high-resolution spectra of 28 A and 22 F stars in the Kepler field, observed with the FIES spectrograph at the Nordic Optical Telescope. We provide spectral types, atmospheric parameters and chemical abundances for 50 stars. Balmer,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4cf03299160bae6b78967b35147fbd13
http://arxiv.org/abs/1707.00613
http://arxiv.org/abs/1707.00613
Autor:
Juan Fabregat, Maryline Briquet, Monica Rainer, Yves Fremat, K. Uytterhoeven, Coralie Neiner, Juan Carlos Suárez, Marcelo Emilio, Eduardo Janot-Pacheco, L. Andrade, P. D. Diago, Ennio Poretti, P. Mathias, Juan Gutiérrez-Soto
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2017, 603, pp.A41. ⟨10.1051/0004-6361/201629177⟩
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. 2017 Photometric and spectroscopic variability of the B5IIIe star HD 171219 Astronomy and Astrophysics 603 A41
RODERIC. Repositorio Institucional de la Universitat de Valéncia
instname
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 603, pp.A41. ⟨10.1051/0004-6361/201629177⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Digital.CSIC. Repositorio Institucional del CSIC
Astronomy and Astrophysics-A&A, 2017, 603, pp.A41. ⟨10.1051/0004-6361/201629177⟩
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. 2017 Photometric and spectroscopic variability of the B5IIIe star HD 171219 Astronomy and Astrophysics 603 A41
RODERIC. Repositorio Institucional de la Universitat de Valéncia
instname
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 603, pp.A41. ⟨10.1051/0004-6361/201629177⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Digital.CSIC. Repositorio Institucional del CSIC
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c06c7df9c94564b44fd48fcf4c5ce95f
https://hal-obspm.ccsd.cnrs.fr/obspm-02268061
https://hal-obspm.ccsd.cnrs.fr/obspm-02268061
Publikováno v:
Astronomical Review. 9:41-65
As part of the NASA Kepler Guest Observer program, we requested and obtained long-cadence data on about 2700 faint (magnitude 14-16) Kepler stars with effective temperatures and surface gravities that lie near or within the pulsation instability regi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9b21b15fe9d26a7476226909da3f070
https://doi.org/10.1080/21672857.2014.11519730
https://doi.org/10.1080/21672857.2014.11519730
Autor:
K. Uytterhoeven
Publikováno v:
Proceedings of the International Astronomical Union. 9:101-107
Time-series of high-resolution spectra of massive main-sequence pulsators contain information on the degree l and azimuthal number m of a pulsation mode. I present an overview of existing mode-identification techniques that have been developed to der
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0333dda0feeac2e1706a05407b55749b
https://doi.org/10.1017/s1743921313014166
https://doi.org/10.1017/s1743921313014166
Publikováno v:
Proceedings of the International Astronomical Union. 9:63-66
We examine the light curves of over 2700 stars observed in long cadence by the Kepler spacecraft as part of the Guest Observer program. Most of these stars are faint (Kepler magnitude > 14), and fall near or within the effective temperature and log g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cf0b8433ead2cbd791539e7ba414b347
https://doi.org/10.1017/s1743921313014099
https://doi.org/10.1017/s1743921313014099
Autor:
P. De Cat, L. A. Balona, Giovanni Catanzaro, K. Uytterhoeven, L. Crause, Davide Gandolfi, Petr Kabath, Margarida S. Cunha, A. P. Hatzes
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 432:2808-2817
KIC 8677585 is a roAp star in the Kepler field which is unique in that there are four lowfrequency variations of unknown origin in addition to more than twenty high-frequency roAp modes. We analysed all available spectroscopy and conclude that the st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::779a4274d7cfb6d49f8cb93265758baf
https://doi.org/10.1093/mnras/stt636
https://doi.org/10.1093/mnras/stt636