Astronomy and Astrophysics – Astronomy
Scientific paper
May 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.5310a&link_type=abstract
American Astronomical Society, 194th AAS Meeting, #53.10; Bulletin of the American Astronomical Society, Vol. 31, p.906
Astronomy and Astrophysics
Astronomy
Scientific paper
We present Hubble Space Telescope observations of four elliptical galaxies out to the distance of the Coma cluster. We recently acquired four single orbit pointings of each of the four galaxies using the F160W filter with NICMOS to cover most of the Planetary Camera field of archival WFPC2 V-band images of the same galaxies. The V-H color index yields sensitive metallicity distributions of the globular clusters systems (GCSs), and it is about three times as sensitive as the V-I color index with a low sensitivity to age variations. We expect the precision of these metallicities to be as good as 0.2 dex. In addition to the GCS metallicity distributions, the H-band observations of the two ellipticals in Coma provide sufficient signal-to-noise to provide good measurements of their H-band surface brightness fluctuation (SBF) amplitudes. We present a preliminary distance to the Coma cluster from the H-band SBF measurements of the two galaxies and briefly discuss its implications on the Hubble constant.
Ajhar Edward A.
Elias Juan
Geisler Doug
Hoard Don
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