Samenvatting
We show that the D(n)-sigma relation, used for estimating distances to elliptical galaxies, needs a surface brightness correction. This correction follows from the universality of the R1/4 law, and can be derived analytically. It resolves the surface brightness bias problem of the D(n)-sigma relation noted earlier.
Originele taal-2 | English |
---|---|
Pagina's (van-tot) | 627-630 |
Aantal pagina's | 4 |
Tijdschrift | Monthly Notices of the Royal Astronomical Society |
Volume | 265 |
Nummer van het tijdschrift | 3 |
Status | Published - 1-dec.-1993 |