000002510 001__ 2510
000002510 005__ 20160701171706.0
000002510 037__ $$aASTROimport-667
000002510 100__ $$aHensberge, H.
000002510 245__ $$aHD 123335, an interesting eclipsing SB2 in Centaurus
000002510 260__ $$c2004
000002510 520__ $$aNew extensive differential uvby photometry at the Danish SAT telescope, and high-resolution spectroscopy at ESO, SAAO and Mt. John Observatory reveal that HD 123335 (HR 5292) is an eclipsing SB2 consisting of two sharp-lined B-type stars in an eccentric orbit (e = 0.735, Porb = 35.44735 deg). The slowest rotating component (Prot = 61.46 deg) is a chemically peculiar (CP) star of the type He-weak SrTi. 
000002510 700__ $$a Nitschelm, C.
000002510 700__ $$a Freyhammer, L. M.
000002510 700__ $$a Bouzid, M. Y.
000002510 700__ $$a Clausen, J. V.
000002510 700__ $$a David, M.
000002510 700__ $$a Helt, B. E.
000002510 700__ $$a Olsen, E. H.
000002510 700__ $$a Papadaki, C.
000002510 700__ $$a Sterken, C.
000002510 700__ $$a Vaz, L. P. R.
000002510 773__ $$c309-311$$pSpectroscopically and Spatially Resolving the Components of the Close Binary Stars$$v318$$y2004
000002510 85642 $$ahttp://esoads.eso.org/abs/2004ASPC..318..309H
000002510 905__ $$apublished in
000002510 980__ $$aNONREF