Astron. Astrophys. Suppl. Ser.
Volume 125, Number 2, October II 1997
|Page(s)||255 - 261|
|Published online||15 October 1997|
Calibration of the Tully-Fisher relation in the field
ANPE and Centre de Physique Théorique, CNRS, Luminy Case 907, F-13288 Marseille Cedex 9, France
Send offprint request to: S. Rauzy
Accepted: 20 December 1996
A new technique for calibrating slope and relative zero-point of Tully-Fisher like relations by using a sample of distant field galaxies is proposed. Based on a null-correlation approach (NCA), the technique is insensitive to the presence of selection effects on apparent magnitude m and on log line-width distance indicator p. This interesting property is used for discarding nearby galaxies of the observed sample. It is shown that such a subsampling allows in effect to attenuate biases on calibration parameters created by the presence of radial peculiar velocities.
Key words: galaxies: distances and redshifts / distance scale
© European Southern Observatory (ESO), 1997