Astron. Astrophys. Suppl. Ser.
Volume 128, Number 1, February II 1998
|Page(s)||29 - 33|
|Published online||15 February 1998|
X-ray/optical observations of stars with shallow convection zones *
Astronomical Institute "Anton Pannekoek" / CHEAF, Kruislaan 403, NL-1098 SJ Amsterdam, The Netherlands
2 Physics Department UAH, Huntsville, AL 35899, U.S.A.
3 Max Planck Institut für Extraterrestrische Physik, Giessenbachstraße 1, 8046 Garching bei München, Germany
Send offprint request to: J. van Paradijs
Accepted: 16 June 1997
We present Walraven photometry and ROSAT All-Sky Survey data for a sample of 173 bright main-sequence stars with spectral types between A8V and G2V. These observations are part of a study of the onset of magnetic surface activity along the main sequence. Values for the effective temperature, surface gravity and interstellar reddening have been obtained from a comparison of the observed Walraven colours with theoretical values. These parameters have been used to derive accurate surface flux densities.
Key words: stars: activity; fundamental parameters / X-rays: stars
Tables 1, 2 and 5 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (220.127.116.11) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1998