Detection of solar-like oscillations in the bright red giant stars γ Piscium and θ1 Tauri from a 190-day high-precision spectroscopic multi-site campaign
dc.contributor.author | Beck, P.G. | |
dc.contributor.author | Kambe, E. | |
dc.contributor.author | Hillen, M. | |
dc.contributor.author | Corsaro, E. | |
dc.contributor.author | Van Winckel, H. | |
dc.contributor.author | Moravveji, E. | |
dc.contributor.author | De Ridder, J. | |
dc.contributor.author | Bloemen, S. | |
dc.contributor.author | Saesen, S. | |
dc.contributor.author | Mathias, P. | |
dc.contributor.author | Degroote, P. | |
dc.contributor.author | Kallinger, T. | |
dc.contributor.author | Verhoelst, T. | |
dc.contributor.author | Ando, H. | |
dc.contributor.author | Carrier, F. | |
dc.contributor.author | Acke, B. | |
dc.contributor.author | Oreiro, R. | |
dc.contributor.author | Miglio, A. | |
dc.contributor.author | Eggenberger, P. | |
dc.contributor.author | Sato, B. | |
dc.contributor.author | Zwintz, K. | |
dc.contributor.author | Papics, P.I. | |
dc.contributor.author | Marcos-Arenal, P. | |
dc.contributor.author | Sans Fuentes, S.A. | |
dc.contributor.author | Schmid, V.S. | |
dc.contributor.author | Waelkens, C. | |
dc.contributor.author | Ostensen, R. | |
dc.contributor.author | Matthews, J.M. | |
dc.contributor.author | Yoshida, M. | |
dc.contributor.author | Izumiura, H. | |
dc.contributor.author | Koyano, H. | |
dc.contributor.author | Nagayama, S. | |
dc.contributor.author | Shimizu, Y. | |
dc.contributor.author | Okada, N. | |
dc.contributor.author | Okita, K. | |
dc.contributor.author | Sakamoto, A. | |
dc.contributor.author | Yamamuro, T. | |
dc.contributor.author | Aerts, C. | |
dc.date | 2015 | |
dc.date.accessioned | 2016-03-24T09:51:23Z | |
dc.date.available | 2016-03-24T09:51:23Z | |
dc.identifier.uri | https://orfeo.belnet.be/handle/internal/2705 | |
dc.language | eng | |
dc.title | Detection of solar-like oscillations in the bright red giant stars γ Piscium and θ1 Tauri from a 190-day high-precision spectroscopic multi-site campaign | |
dc.type | Article | |
dc.subject.frascati | Physical sciences | |
dc.audience | Scientific | |
dc.subject.free | Astronomy | |
dc.subject.free | Geometrical optics | |
dc.subject.free | Interferometry | |
dc.subject.free | Seismology | |
dc.subject.free | Separation | |
dc.subject.free | Stars | |
dc.subject.free | Velocity | |
dc.subject.free | Asteroseismology | |
dc.subject.free | Stars: general | |
dc.subject.free | Stars: Rotation | |
dc.subject.free | Techniques: interferometric | |
dc.subject.free | Techniques: spectroscopic | |
dc.subject.free | Giant stars | |
dc.source.title | Astronomy and Astrophysics | |
dc.source.volume | 573 | |
dc.source.page | A138 | |
Orfeo.peerreviewed | Yes | |
dc.identifier.doi | 10.1051/0004-6361/201323019 | |
dc.identifier.scopus | 2-s2.0-84921326784 |