000002048 001__ 2048
000002048 005__ 20160701171657.0
000002048 0247_ $$2DOI$$a10.1553/cia147s52
000002048 037__ $$aASTROimport-205
000002048 100__ $$aCuypers, J.
000002048 245__ $$aAnalysis of MERCATOR data - Part II: variable A  F stars
000002048 260__ $$c2006
000002048 520__ $$aFor a few decades, a large international community is working at the development of stellar seismology, intending to open a new window on the structure and evolution of stars, with the necessary parallel development of new observational techniques, modeling tools and methods for diagnostics and interpretation. This new window is associated with new observables, characterizing the oscillations (frequencies, amplitudes, line profiles,...) which are sensitive to the stellar interior and thus very complementary with surface observables, associated to astrometry, spectropolarimetry or interferometry. 
000002048 700__ $$a Goossens, K.
000002048 700__ $$a Schoenaers, C.
000002048 700__ $$a De Cat, P.
000002048 700__ $$a Aerts, C.
000002048 773__ $$c52-55$$pCommunications in Asteroseismology$$v147$$y2006
000002048 85642 $$ahttp://esoads.eso.org/abs/2006CoAst.147...52C
000002048 905__ $$apublished in
000002048 980__ $$aREFERD