1998/09/17 by Carl J. Grillmair, Duncan A. Forbes, Jean P. Brodie +2 · 1 citation
Physics and Astronomy · #Advanced Camera for Surveys #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Elliptical galaxy #Fornax Cluster #Galaxies: Formation, Evolution, Phenomena #Galaxy #Globular cluster #Hubble Deep Field #Hubble Ultra-Deep Field #Hubble space telescope #Intergalactic travel #Luminosity #Luminosity function #Physics #Redshift #Stellar, planetary, and galactic studies #Virgo Cluster #astro-ph
paper · pdf · doi:10.1086/300661
32 pages, incl. 2 JPEG figures, AAS LaTeX, to be published in the Astronomical Journal
arxiv created 1998/09/17 · openalex publication_date 1999/01/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We examine the luminosity and B - I color distribution of globular clusters for three early-type galaxies in the Fornax Cluster using imaging data from the Wide Field Planetary Camera 2 on the Hubble Space Telescope . The luminosity functions we derive are in most cases better than 50% complete down to B = 26.6. We find that the color distributions of globular clusters in the central region of NGC 1399 and its nearby neighbor NGC 1404 are bimodal and statistically indistinguishable. The metallicity spread, as inferred from the color distributions in these two galaxies, is very similar to that of M87. NGC 1399's luminosity function is also very similar to that of M87, and comparing their respective peak magnitudes indicates that the Fornax Cluster is at very nearly the same distance from the Local Group as is the Virgo Cluster. From this we derive H 0 = 82 ± 8 km s -1 Mpc -1 , where the uncertainty reflects only the effects of random errors. The number of unresolved objects we find at a projected distance of 440 kpc from NGC 1399 is consistent with nothing more than compact background galaxies, though the small field of view of the WFPC2 does not allow us to put strong constraints on the number of intergalactic globular clusters. The luminosity function of objects detected around NGC 1316 is more nearly exponential than lognormal, and both the color and size distribution of these objects distinguish them from the clusters surrounding NGC 1399. We suggest that these objects are more akin to old open clusters in the Galaxy than they are to globular clusters in typical early-type galaxies.