000002583 001__ 2583
000002583 005__ 20160701171707.0
000002583 0247_ $$2DOI$$a10.1007/978-3-540-74745-1_7
000002583 037__ $$aASTROimport-740
000002583 100__ $$aHensberge, H.
000002583 245__ $$aSpectral Disentangling Applied to Triple Systems: RV Crt
000002583 260__ $$c2008
000002583 520__ $$aThe eclipsing triple system RV Crt shows a composite spectrum dominated by the sharp-lined late-F type spectrum of the tertiary. The spectral lines of the close binary are considerably broadened, since both components rotate synchronously with the orbit. The Doppler shifts and the component spectra are successfully recovered by application of the spectral disentangling technique. The cooler, less massive component of the close binary is larger than the hotter one. The hotter component of the close binary is very similar to the tertiary. The system is probably still on its way to the zero-age main sequence 
000002583 700__ $$a Vaz, L. P. R.
000002583 700__ $$a Torres, K. B. V.
000002583 700__ $$a Armond, T.
000002583 773__ $$c47$$pMultiple Stars Across the H-R Diagram$$y2008
000002583 85642 $$ahttp://esoads.eso.org/abs/2008msah.conf...47H
000002583 905__ $$apublished in
000002583 980__ $$aNONREF