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000001917 0247_ $$2DOI$$a10.1051/0004-6361:20011406
000001917 037__ $$aASTROimport-74
000001917 100__ $$aMathias, P.
000001917 245__ $$aSpectroscopic monitoring of 10 new northern slowly pulsating B star candidates discovered from the HIPPARCOS mission
000001917 260__ $$c2001
000001917 520__ $$aA one-year follow-up campaign of high-resolution, high-signal-to-noise spectroscopy for 10 candidate slowly pulsating B stars, which were discovered from the HIPPARCOS astrometric mission, shows that all stars exhibit line-profile variability. From our data, and from the HIPPARCOS photometry, we conclude that all but one of the targets provide evidence of multiperiodicity, with periods of the order of days, confirming their pulsational nature. Thus they are confirmed slowly pulsating B stars. We summarize the pulsation periods and Q-values and select the most interesting targets for very-long-term follow-up observations with the goal of performing asteroseismology. Based on observations obtained at the Observatoire de Haute-Provence. 
000001917 700__ $$a Aerts, C.
000001917 700__ $$a Briquet, M.
000001917 700__ $$a De Cat, P.
000001917 700__ $$a Cuypers, J.
000001917 700__ $$a Van Winckel, H.
000001917 700__ $$a Le Contel, J. M.
000001917 773__ $$c905-916$$pAstronomy and Astrophysics$$v379$$y2001
000001917 85642 $$ahttp://esoads.eso.org/abs/2001A%26A...379..905M
000001917 905__ $$apublished in
000001917 980__ $$aREFERD