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2014MNRAS.438.3535S - Mon. Not. R. Astron. Soc., 438, 3535-3556 (2014/March-2)
Extensive study of HD 25558, a long-period double-lined binary with two SPB components.
SODOR A., DE CAT P., WRIGHT D.J., NEINER C., BRIQUET M., LAMPENS P., DUKES R.J., HENRY G.W., WILLIAMSON M.H., BRUNSDEN E., POLLARD K.R., COTTRELL P.L., MAISONNEUVE F., KILMARTIN P.M., MATTHEWS J., KALLINGER T., BECK P.G., KAMBE E., ENGELBRECHT C.A., CZANIK R.J., YANG S., HASHIMOTO O., HONDA S., FU J.N., CASTANHEIRA B., LEHMANN H., BOGNAR Zs., BEHARA N., SCARINGI S., VAN WINCKEL H., MENU J., LOBEL A., MATHIAS P., SAESEN S., VUCKOVIC M. (The MiMeS Collaboration)
Abstract (from CDS):
Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)
Journal keyword(s): asteroseismology - binaries: spectroscopic - stars: individual: HD 25558 - stars: magnetic field - stars: oscillations - stars: rotation
Simbad objects: 6
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