Institut für Astronomie, Universität Wien,
Türkenschanzstraße 17, A-1180 Wien, Austria
e-mail: name@astro.univie.ac.at
We present the results from a spectroscopic Ca
II H&K survey
of 1058 late-type stars selected from a color-limited subsample of the
Hipparcos catalog. Out of these 1058 stars, 371 stars were found to
show significant H&K emission, most of them previously unknown;
23% with strong emission, 36% with moderate emission, and
41% with weak emission. These spectra are used to determine
absolute H&K emission-line fluxes, radial velocities, and equivalent
widths of the luminosity-sensitive Sr
II line at 4077 Å.
Red-wavelength spectroscopic and Strömgren
y photometric follow-up
observations of the 371 stars with H&K emission are used to
additionally determine the absolute H

-core flux, the lithium
abundance from the Li
I 6708 Å equivalent width, the rotational
velocity

,
the radial velocity, and the light variations and its
periodicity. The latter is interpreted as the stellar rotation period due
to an inhomogeneous surface brightness distribution. 156 stars were found
with photometric periods between 0.29 and 64 days, 11 additional systems
showed quasi-periodic variations possibly in excess of

50 days.
Further 54 stars had variations but no unique period was found, and four
stars were essentially constant.
Altogether, 170 new variable stars were discovered. Additionally,
we found 17 new SB1 (plus 16 new candidates) and 19 new SB2 systems,
as well as one definite and two possible new SB3 systems.
Finally, we present a list of 21 stars that we think are most suitable
candidates for a detailed study with the Doppler-imaging technique.
Key words: stars: activity -- stars: chromospheres --
stars: late-type -- stars: rotation -- surveys