Astron. Astrophys. 359, 1059-1067 (2000)

Footnotes

1. Average values with log 1.0-1.5.

2. , with .

3. For sake of homogeneity, we adopt the Cepheid distances listed in Ferrarese et al. (1999).

© European Southern Observatory (ESO) 2000

Online publication: July 13, 2000
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