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相关论文: The Globular Cluster Systems in the Coma Elliptica…

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Shells in Elliptical Galaxies are faint, sharp-edged features, believed to provide evidence of a recent ($\sim 0.5 - 2 \times 10^9$ years ago) merger event. We analyse the Globular Cluster (GC) systems of six shell elliptical galaxies, to…

天体物理学 · 物理学 2009-11-11 G. Sikkema , R. F. Peletier , D. Carter , E. A. Valentijn , M. Balcells

A dataset of 23,351 globular clusters (GCs) and ultra-compact dwarfs (UCDs) in the Coma cluster of galaxies was built using Hubble Space Telescope Advanced Camera for Surveys data. Based on the standard magnitude cut of $M_V \leq -11$, a…

星系天体物理 · 物理学 2025-07-22 Richard T. Pomeroy , Juan P. Madrid , Conor R. O'Neill , Alexander T. Gagliano

We study the globular cluster system (GCS) of the giant elliptical NGC4374 (M84) in the Virgo cluster using B and R photometry. The colour distribution is bimodal with peaks at B-R=1.11 and B-R=1.36, fitting well to those found in other…

天体物理学 · 物理学 2009-11-10 M. Gomez , T. Richtler

Nearby massive compact elliptical galaxies (MCEGs) are strong candidates for relic galaxies (i.e. local analogs of red nuggets at high redshifts). It is expected that the globular cluster (GC) systems of relic galaxies are dominated by red…

星系天体物理 · 物理学 2021-06-23 Jisu Kang , Myung Gyoon Lee

CFHT Megacam data in (g',r',i') are used to obtain deep, wide-field photometry of the globular cluster system (GCS) around M87. A total of 6200 GCs brighter than M_I = -8.5 are included in the study, essentially containing almost the entire…

星系天体物理 · 物理学 2015-05-13 William E. Harris

We present a kinematic analysis of the globular cluster (GC) system in the giant elliptical galaxy (gE) M60 in the Virgo cluster. Using the photometric and spectroscopic database of 121 GCs (83 blue GCs and 38 red GCs), we have investigated…

We use data from the HST Coma Cluster Treasury program to assess the richness of the Globular Cluster Systems (GCSs) of 54 Coma ultra-diffuse galaxies (UDGs), 18 of which have a half-light radius exceeding 1.5 kpc. We use a hierarchical…

星系天体物理 · 物理学 2018-07-18 N. C. Amorisco , A. Monachesi , A. Agnello , S. D. M. White

We study the globular cluster (GC) system of the Virgo giant elliptical galaxy NGC 4365, using new wide-field VIK imaging. The GC colour distribution has (at least) two peaks, but the colours of the red GCs appear more strongly weighted…

天体物理学 · 物理学 2009-11-11 S. S. Larsen , J. P. Brodie , J. Strader

We present a study of the colors of globular clusters associated with the elliptical galaxy NGC 3923. Our final sample consists of Washington system C and T_1 photometry for 143 globular cluster candidates with an expected contamination of…

天体物理学 · 物理学 2009-10-22 Stephen E. Zepf , Keith M. Ashman , Doug Geisler

The Coma cluster is one of the richest known cluster of galaxies, spanning about 4 dex in density. Hence it is the ideal place to study the structure of galaxies as a function of environmental density in order to constrain the theories of…

天体物理学 · 物理学 2007-05-23 Doerte Mehlert , Roberto P. Saglia , Ralf Bender , Gary Wegner

We present a kinematic analysis of the globular cluster(GC) system in the giant elliptical galaxy (gE) NGC 4636 in the Virgo cluster. Using the photometric and spectroscopic database of 238 GCs, we have investigated the kinematics of the GC…

宇宙学与河外天体物理 · 物理学 2014-11-20 Myung Gyoon Lee , Hong Soo Park , Ho Seong Hwang , Nobuo Arimoto , Naoyuki Tamura , Masato Onodera

This paper presents results from wide-field imaging of the globular cluster (GC) systems of five intermediate-luminosity (M_V ~-21 to -22) early-type galaxies. The aim is to accurately quantify the global properties of the GC systems by…

宇宙学与河外天体物理 · 物理学 2015-06-11 Jonathan R. Hargis , Katherine L. Rhode

In this work we perform the photometric analysis of the globular cluster system (GCS) of the giant elliptical NGC4696, which is the brightest member of Centaurus, a rich and dynamically young galaxy cluster. We obtained deep Magellan 6.5…

星系天体物理 · 物理学 2024-09-25 S. Federle , M. Gómez , S. Mieske , W. E. Harris , M. Hilker , I. A. Yegorova , G. L. H. Harris

Bimodality is a common feature of globular cluster (GC) color distributions in galaxies. Although it is well known that the GC system of the Milky Way is bimodal in metallicity, this has yet to be directly demonstrated for an elliptical…

天体物理学 · 物理学 2008-11-26 Jay Strader , Michael A. Beasley , Jean P. Brodie

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…

星系天体物理 · 物理学 2016-10-12 Michael A. Beasley , Ignacio Trujillo

1057 globular cluster candidates have been identified in a WFPC2 image of the inner region of M87. The Globular Cluster Luminosity Function (GCLF) can be well fit by a Gaussian profile with a mean value of m_V^0=23.67 +/- 0.07 mag and…

天体物理学 · 物理学 2009-10-05 A. Kundu , B. C. Whitmore , W. B. Sparks , F. D. Macchetto , S. E. Zepf , K. M. Ashman

We present a new photometric catalogue of the rich globular cluster (GC) system around M87, the brightest cluster galaxy in Virgo. Using archival Next Generation Virgo cluster Survey (NGVS) images in the ugriz bands, observed with…

星系天体物理 · 物理学 2015-11-24 L. J. Oldham , M. W. Auger

We present a photometric study of the globular clusters in the giant elliptical galaxy M60 in the Virgo cluster, based on deep, relatively wide field Washington CT_1 CCD images. The color-magnitude diagram reveals a significant population…

天体物理学 · 物理学 2010-11-11 Myung Gyoon Lee , Hong Soo Park , Eunhyeuk Kim , Ho Seong Hwang , Sang Chul Kim , Doug Geisler

We study the Globular Cluster (GC) system of the nearby elliptical galaxy M87 using the newly available dataset with accurate kinematics (Strader et al.2011). We find evidence for three distinct sub-populations of GCs in terms of colours,…

星系天体物理 · 物理学 2015-06-18 A. Agnello , N. W. Evans , A. J. Romanowsky , J. P. Brodie

We have assembled a large data-set of 613 galaxy redshifts in the Coma cluster, the largest presently available for a cluster of galaxies. We have defined a sample of cluster members complete to b$_{26.5}=20.0$, using a membership criterion…

天体物理学 · 物理学 2007-05-23 A. Biviano , F. Durret , D. Gerbal , O. LeFevre , C. Lobo , A. Mazure , E. Slezak