المؤلفون: Matt A. Wood, Donald E Winget, E. W. Klumpe, R. E. Nather, Christophe Massacand, S. Hemar, T. M. K. Marar, G. Vauclair, Denis J. Sullivan, E. G. Meištas, O. Giovannini, J. Krzesinski, B. C. Bhat, Antonio Kanaan, V. C. Babu, Judith L. Provencal, P. Ibbetson, S. J. Kleinman, Paul A. Bradley, B. N. Ashoka, G. Pajdosz, E. Mashals, Staszek Zola, M. S. O’Brien, D. A. H. Buckley, H. S. Mahra, T. K. Watson, Michael H. Montgomery, Kinwah Wu, François Vuille, Elia M. Leibowitz, S. Seetha, Souza Oliveira Kepler, D. O'Donoghue, Pawel Moskalik, A. Nitta, J. E. Solheim, J. C. Clemens, S. Bard

المصدر: Monthly Notices of the Royal Astronomical Society. 314:689-701

مصطلحات موضوعية: Data set, Physics, Total harmonic distortion, Amplitude, Space and Planetary Science, Normal mode, Mode (statistics), White dwarf, Astronomy and Astrophysics, Astrophysics, Star (graph theory), Spectral line

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_________::49039cc137b395c08042fa045525cda9
https://doi.org/10.1046/j.1365-8711.2000.03369.x