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The optical colors of globular clusters (GCs) in most large early-type galaxies are bimodal. Blue and red GCs show a sharp difference in the radial profile of their surface number density in the sense that red GCs are more centrally…

Astrophysics of Galaxies · Physics 2021-01-06 Sang-Yoon Lee , Chul Chung , Suk-Jin Yoon

We present wide-field multiband photometry of globular cluster (GC) systems in NGC 1399, NGC 1404, and NGC 1387 located at the central region of the Fornax galaxy cluster. Observation was carried out through U, B, V, and I bands, which…

Astrophysics of Galaxies · Physics 2015-06-12 Hak-Sub Kim , Suk-Jin Yoon , Sangmo Tony Sohn , Sang Chul Kim , Eunhyeuk Kim , Chul Chung , Sang-Yoon Lee , Young-Wook Lee

Here we present HST/ACS imaging, in the B and I bands, of the edge-on Sb/Sc galaxy NGC 5170. Excluding the central disk region region, we detect a 142 objects with colours and sizes typical of globular clusters (GCs). Our main result is the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Duncan Forbes , Lee Spitler , William Harris , Jeremy Bailin , Jay Strader , Jean Brodie , Soeren Larsen

Using Magellan/IMACS images covering a 1.2 x 1.2 sq. degree FOV with seeing of 0.4"-0.6", we have applied convolution techniques to analyse the light distribution of 364 confirmed globular cluster in the field of NGC 5128 and to obtain…

Astrophysics · Physics 2009-11-13 M. Gomez , K. A. Woodley

(Abridged) We measure the mass distribution of galaxy cluster Abell 1689 within 0.3 Mpc/h_70 of the cluster centre using its strong lensing effect on 32 background galaxies. The multiple images are based on those of Broadhurst et al. 2005…

Astrophysics · Physics 2009-11-11 A. Halkola , S. Seitz , M. Pannella

NGC 5846 is a giant elliptical galaxy with a previously well studied globular cluster system (GCS), known to have a bimodal colour distribution with a remarkably high red fraction. Here we revisit the central galaxy regions searching for…

Astrophysics · Physics 2009-11-11 A. L. Chies-Santos , M. G. Pastoriza , B. X. Santiago , D. A. Forbes

We present a preliminary analysis of HST-WFPC2 observations of globular cluster systems in the two brightest galaxies, UGC 9799 (cD) and NGC 1129 (non-cD), located in the center of rich clusters.

Astrophysics · Physics 2007-05-23 Myung Gyoon Lee , Eunhyeuk Kim , Doug Geisler , Terry Bridges , Keith Ashman

Color-magnitude diagrams (CMDs) derived from Hubble Space Telescope (HST) Advanced Camera for Surveys F606W,F814W photometry of 6 globular clusters (GCs) are presented. The six GCs form two loose groupings in Galactocentric distance (Rgc):…

Astrophysics of Galaxies · Physics 2015-05-28 Aaron Dotter , Ata Sarajedini , Jay Anderson

We study the globular cluster (GC) system of the dust-lane elliptical galaxy NGC 6702, using B, V and I-band photometric observations carried out at the Keck telescope. This galaxy has a spectroscopic age of ~2Gyrs suggesting recent…

Astrophysics · Physics 2009-10-31 A. Georgakakis , D. A. Forbes , J. P. Brodie

We present new HST/WFPC2 (V,I) photometry for the red-giant stars in NGC 5128 at a projected distance of 8 kpc from the galaxy center, which probe a mixture of its inner halo and outer bulge. The color-magnitude diagram shows an old…

Astrophysics · Physics 2009-11-07 W. E. Harris , G. L. H. Harris

We present an analysis of archival {\it HST/ACS} imaging in the F475W ($g_{475}$), F606W ($V_{606}$) and F814W ($I_{814}$) bands of the globular cluster (GC) system of a large (3.4 kpc effective radius) ultra-diffuse galaxy (DF17) believed…

Astrophysics of Galaxies · Physics 2016-10-12 Michael A. Beasley , Ignacio Trujillo

We present internal surface-brightness profiles, based on HST/ACS imaging in the F606W bandpass, for 131 globular cluster (GC) candidates with luminosities 10^4 - 3 x 10^6 solar, in the giant elliptical galaxy NGC 5128. Several structural…

We present a study of globular clusters (GCs) in 17 relatively nearby early-type galaxies, based on deep HST/WFPC2 F555W and F814W images. We compare color distributions, cluster sizes and luminosity functions with those of GCs in the Milky…

Astrophysics · Physics 2008-11-26 S. S. Larsen , J. P. Brodie , J. P. Huchra , D. A. Forbes , C. Grillmair

We present a wide-field study of the globular cluster systems (GCS) of the elliptical galaxy NGC 3640 and its companion NGC 3641, based on observations from Gemini Multi-Object Spectrograph/Gemini using the g'r'i' filters. NGC 3640 is a…

Astrophysics of Galaxies · Physics 2024-10-16 Ana Ines Ennis , Juan Pablo Caso , Lilia Patricia Bassino

We present the first results from our HST Brightest Cluster Galaxy (BCG) survey of seven central supergiant cluster galaxies and their globular cluster (GC) systems. We measure a total of 48000 GCs in all seven galaxies, representing the…

We study the quiescent ultra-diffuse galaxy FCC 224 in the Fornax cluster using Hubble Space Telescope (HST) imaging, motivated by peculiar properties of its globular cluster (GC) system revealed in shallower imaging. The surface brightness…

We present the results of a photometric study of the early-type galaxy NGC 6876 and the surrounding globular cluster system (GCS). The host galaxy is a massive elliptical, the brightest of this type in the Pavo Group. According to its…

Astrophysics of Galaxies · Physics 2019-07-05 Ana Inés Ennis , Lilia Patricia Bassino , Juan Pablo Caso , Bruno Javier De Bórtoli

We present photometry for the globular cluster NGC 6642 using the F606W and F814W filters with the ACS/WFC third generation camera on board of Hubble Space Telescope. The Colour Magnitude Diagram shows sources reaching ~ 6 mags below the…

Astrophysics of Galaxies · Physics 2015-05-13 E. Balbinot , B. X. Santiago , E. Bica , C. Bonatto

We study the globular cluster (GC) populations of 21 giant elliptical galaxies in 19 Abell clusters. This method, applied here primarily in the R band, is based on the surface brightness fluctuations technique of extragalactic distance…

Astrophysics · Physics 2009-10-30 John P. Blakeslee , John L. Tonry , Mark R. Metzger

We present Gemini griz photometry for 521 globular cluster (GC) candidates in a 5.5 x 5.5 arcmin field centered 3.8 arcmin to the south and 0.9 arcmin to the west of the center of the giant elliptical galaxy NGC 4486. All these objects have…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Juan C. Forte , Favio R. Faifer , E. Irene Vega , Lilia P. Bassino , Analia V. Smith Castelli , Sergio A. Cellone , Douglas Geisler
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