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Related papers: Multicolour-metallicity Relations from Globular Cl…

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Studies based on Hubble Space Telescope ($HST$) photometry in F275W, F336W, and F438W have shown that the incidence and complexity of multiple populations (MPs) in Globular Clusters (GCs) depend on cluster mass. This result, however, is…

Solar and Stellar Astrophysics · Physics 2020-01-08 Edoardo P. Lagioia , Antonino P. Milone , Anna F. Marino , Giacomo Cordoni , Marco Tailo

We perform aperture photometry and profile fitting on 419 globular cluster (GC) candidates with mV \leq 23 mag identified in Hubble Space Telescope Advanced Camera for Surveys BVI imaging, and estimate the effective radii of the clusters.…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Julie B. Nantais , John P. Huchra , Andreas Zezas , Kosmas Gazeas , Jay Strader

We combine new Wide Field Camera~3 IR Channel (WFC3/IR) F160W (H) imaging data for NGC1399, the central galaxy in the Fornax cluster, with archival F475W (g), F606W (V), F814W (I), and F850LP (z) optical data from the Advanced Camera for…

Cosmology and Nongalactic Astrophysics · Physics 2012-02-01 John P. Blakeslee , Hyejeon Cho , Eric W. Peng , Laura Ferrarese , Andres Jordan , Andre R. Martel

We compare optical and near infrared colours of globular clusters in M87, the central giant elliptical in Virgo, and NGC 4478, an intermediate luminosity galaxy in Virgo, close in projection to M87. Combining V and I photometry obtained…

Astrophysics · Physics 2009-11-07 Markus Kissler-Patig , Jean P. Brodie , Dante Minniti

We present the first results from the GeMS/GSAOI Galactic Globular Cluster Survey (G4CS) of the Milky-Way globular clusters (GCs) NGC 3201 and NGC 2298. Using the Gemini South Adaptive Optics Imager (GSAOI), in tandem with the Gemini…

We used deep Gemini-South/GMOS g'r'i'z' images to study the globular cluster (GC) system of the massive elliptical galaxy NGC 1395, located in the Eridanus supergroup. The photometric analysis of the GC candidates reveals a clear colour…

Astrophysics of Galaxies · Physics 2017-12-27 C. G. Escudero , F. R. Faifer , A. V. Smith Castelli , J. C. Forte , L. A. Sesto , N. M. González , M. C. Scalia

We present results from a study of the globular cluster (GC) systems of four spiral and S0 galaxies imaged as part of an ongoing wide-field survey of the GC systems of giant galaxies. The target galaxies -- the SB0 galaxy NGC1023, the SBb…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Michael D. Young , Jessica L. Dowell , Katherine L. Rhode

We present an astrometry and photometry catalogue of globular cluster (GC) candidates detected with HST WFPC2 in a sample of 19 early-type galaxies, appropriate for comparison to the low-mass X-ray binary (LMXB) populations observed with…

Astrophysics · Physics 2008-12-18 Philip J Humphrey

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 wide field JHKs photometry of 16 Galactic globular clusters located towards the Galactic bulge, calibrated on the 2MASS photometric system. Differential reddening corrections and statistical field star decontamination are…

Solar and Stellar Astrophysics · Physics 2016-11-15 Roger E. Cohen , Christian Moni Bidin , Francesco Mauro , Charles Bonatto , Douglas Geisler

We present extensive new photometry in (g',i') of the large globular cluster (GC) system around NGC 3311, the central cD galaxy in the Hydra cluster. Our GMOS data cover a 5.5' field of view and reach a limiting magnitude i' = 26, about 0.5…

Astrophysics · Physics 2009-11-13 Elizabeth Wehner , Bill Harris , Brad Whitmore , Barry Rothberg , Kristin Woodley

We outline a method to measure the detailed chemical composition of extragalactic (unresolved) globular clusters (GCs) from echelle spectra of their integrated light. Our goal is to use this method to measure abundance patterns of GCs in…

Astrophysics · Physics 2007-05-23 R. A. Bernstein , A. McWilliam

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

A detailed imaging analysis of the globular cluster (GC) system of the Sombrero galaxy (NGC 4594) has been accomplished using a six-image mosaic from the Hubble Space Telescope Advanced Camera for Surveys. The quality of the data is such…

Astrophysics · Physics 2008-11-26 L. R. Spitler , S. S. Larsen , J. Strader , J. P. Brodie , D. A. Forbes , M. A. Beasley

Globular Cluster Systems (GCSs) of most early-type galaxies feature two peaks in their optical colour distributions. Blue-peak GCs are believed to be old and metal-poor, whereas the ages, metallicities, and the origin of the red-peak GCs…

Astrophysics · Physics 2009-12-04 R. Kotulla , U. Fritze , P. Anders

Hubble Space Telescope photometry from the ACS/WFC and WFPC2 cameras is used to detect and measure globular clusters (GCs) in the central region of the rich Perseus cluster of galaxies. A detectable population of Intragalactic GCs is found…

Astrophysics of Galaxies · Physics 2017-05-03 William E. Harris , Courtney J. Mulholland

Using the surface brightness fluctuations in HST WFPC-2 images, we determine that M87, NGC 4486B, and NGC 4478 are all at a distance of ~16 Mpc, while NGC 4476 lies in the background at ~21 Mpc. We also examine the globular clusters of M87…

Astrophysics · Physics 2012-08-27 Eric H. Neilsen, , Zlatan I. Tsvetanov , Holland C. Ford

We study the size and structure of globular clusters (GC) systems of 118 early-type galaxies from the NGVS, MATLAS, and ACSVCS surveys. Fitting S\'ersic profiles, we investigate the relationship between effective radii of GC systems ($R_{e,…

Substructure in globular cluster (GC) populations around large galaxies is expected in galaxy formation scenarios that involve accretion or merger events, and it has been searched for using direct associations between GCs and structure in…

We study the globular cluster (GC) systems in three representative fossil group galaxies: the nearest (NGC6482), the prototype (NGC1132) and the most massive known to date (ESO306-017). This is the first systematic study of GC systems in…

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