The mean absolute magnitude of the Am stars was determined from statistical parallaxes. The material comprises 137 Am stars all contained in the “Bright Stars Catalogue”. Separate solution based upon the tau and upsilon components were derived, and both are in excellent agreement. The final value was corrected for an average value of blanketing and for the effect of the invisible spectroscopic companions of the Am stars. The final result is: Mv = 0.9 mag and the mean probable error was estimated to be 0.3 mag. This result locates the Am stars 0.8 mag above the main sequence and 1.5 mag above the ZAMS. The duplicity and the blanketing correction therefore do not modify substantially previous conclusions on the place of the Am stars in the H-...
The spectroscopic absolute magnitudes and parallaxes of 200 A stars have been determined. The materi...
We investigate the light variations of 15 Am stars using four years of high-precision photometry fro...
We sing the praises of the central limit theorem. Having previously removed all other possible cause...
The mean absolute magnitude of the Am stars was determined from statistical parallaxes. The material...
These stellar recounts averaged over all galactic latitudes are analysed by a series of Kapteyn-sche...
We calculate the average absolute magnitude for Hipparcos single K0V stars, using a theoretical curv...
We present absolute magnitude estimates for a number of peculiar star groups, defined on the basis o...
The position of different kinds of CP stars of the upper Main Sequence (i.e. Am stars and the four c...
We combined the (K (s) , J-K (s) ) data in Laney et al. (Mon. Not. R. Astron. Soc. 419:1637, 2012) w...
i. On the relation of mean stellar parallax to proper motion and apparent magnitude • ii. On the p...
As a preliminary step to derive the luminosity function the underlying hypothesis involved in the me...
We sing the praises of the central limit theorem. Having previously removed all other possible cause...
We compare the absolute visual magnitude of the majority of bright O stars in the sky as predicted f...
We analyse a sample of about 500 MK standards of cool spectral types (G to M) for to compare the v...
A re-analysis of the Am star τ U Ma is carried out using new determinations of effective temperature...
The spectroscopic absolute magnitudes and parallaxes of 200 A stars have been determined. The materi...
We investigate the light variations of 15 Am stars using four years of high-precision photometry fro...
We sing the praises of the central limit theorem. Having previously removed all other possible cause...
The mean absolute magnitude of the Am stars was determined from statistical parallaxes. The material...
These stellar recounts averaged over all galactic latitudes are analysed by a series of Kapteyn-sche...
We calculate the average absolute magnitude for Hipparcos single K0V stars, using a theoretical curv...
We present absolute magnitude estimates for a number of peculiar star groups, defined on the basis o...
The position of different kinds of CP stars of the upper Main Sequence (i.e. Am stars and the four c...
We combined the (K (s) , J-K (s) ) data in Laney et al. (Mon. Not. R. Astron. Soc. 419:1637, 2012) w...
i. On the relation of mean stellar parallax to proper motion and apparent magnitude • ii. On the p...
As a preliminary step to derive the luminosity function the underlying hypothesis involved in the me...
We sing the praises of the central limit theorem. Having previously removed all other possible cause...
We compare the absolute visual magnitude of the majority of bright O stars in the sky as predicted f...
We analyse a sample of about 500 MK standards of cool spectral types (G to M) for to compare the v...
A re-analysis of the Am star τ U Ma is carried out using new determinations of effective temperature...
The spectroscopic absolute magnitudes and parallaxes of 200 A stars have been determined. The materi...
We investigate the light variations of 15 Am stars using four years of high-precision photometry fro...
We sing the praises of the central limit theorem. Having previously removed all other possible cause...