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Title: Globular clusters in the inner regions of NGC 5128 (CENTAURUS A)

Journal Article · · Astrophysical Journal
DOI:https://doi.org/10.1086/177597· OSTI ID:388158
 [1];  [2];  [3];  [4];  [3]
  1. Lawrence Livermore National Laboratory, P.O. Box 808, MS L-413, Livermore, California 94551-9900 (United States)
  2. Observatorio Astronomico, Laprida 854, 5000 Cordoba (Argentina)
  3. European Southern Observatory, D-85748 Garching bei Muenchen (Germany)
  4. Observatoire de Paris-Section de Meudon, F-92195 Meudon Cedex (France)

We have identified 26 new globular cluster candidates in the inner 3 kpc of NGC 5128 (Centaurus A), the nearest known large galaxy that is the probable product of a merger. The clusters are selected on the basis of their structural parameters (observed core diameters and ellipticities), as measured from archival Wide Field Planetary Camera (WFPC) {ital Hubble} {ital Space} {ital Telescope} ({ital HST}) images. IR photometry obtained with IRAC2B at the ESO/MPI 2.2 m telescope is combined with the optical HST photometry. Most of these clusters have normal colors typical of old globular clusters like those found in the Milky Way and M31. We estimate their metal abundances based on the {ital R}{minus}{ital K}{sub 0} color, confirming the existence of a metallicity gradient in the inner regions of NGC 5128. The presence of metal-rich globular clusters suggests that one of the colliding galaxies was a bulge-dominated galaxy ({ital E} or early {ital S}). A few clusters have colors and magnitudes similar to intermediate-age clusters containing carbon stars in the Magellanic Clouds. If the intermediate-age clusters were formed during a merger, then this episode must have occurred a few gigayears ago. Alternatively, we are looking at the cluster members of one of the colliding galaxies, which would then have been a late-type disk galaxy. {copyright} {ital 1996 The American Astronomical Society.}

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
388158
Journal Information:
Astrophysical Journal, Vol. 467, Issue 1; Other Information: PBD: Aug 1996
Country of Publication:
United States
Language:
English