Results 121 to 130 of about 59,378 (245)
In this work, we determine the total globular cluster (GC) counts and globular cluster system (GCS) total mass estimates for 27 extremely massive elliptical galaxies.
Veronika Dornan, William E. Harris
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The Manhattan Suite: Accelerated Galaxy Evolution in the Early Universe
Observational advances have allowed the detection of galaxies, protoclusters, and galaxy clusters at higher and higher redshifts, opening a new view into extreme galaxy evolution.
Douglas Rennehan
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Alignment Effects of Brightest Cluster Galaxies [PDF]
D. G. Lambas+2 more
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The Globular Cluster Luminosity Functions of Brightest Cluster Galaxies [PDF]
John P. Blakeslee
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The K-Band Hubble Diagram for the Brightest Cluster Galaxies: A Test of Galaxy Formation Models [PDF]
Alfonso Aragón‐Salamanca+2 more
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We set the stage for reassessing how star formation, emission-line nebulae, and active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs) depend on the thermodynamics of the intracluster medium (ICM).
Arsen Levitskiy+4 more
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A Kinematic Search for Bound Populations around Brightest Cluster Members in a Sample of 52 Clusters of Galaxies [PDF]
D. Bottini
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Spectroscopic and X-ray Modeling of the Strong Lensing Galaxy Cluster MACS J0138.0-2155
We model the total mass and galactic substructure in the strong lensing galaxy cluster MACS J0138.0-2155 using a combination of Chandra X-ray data, Multi-Unit Spectroscopic Explorer (MUSE) spectroscopy, and Hubble Space Telescope imaging.
Abigail Flowers+4 more
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Using Neural Networks to Automate the Identification of Brightest Cluster Galaxies in Large Surveys
Brightest cluster galaxies (BCGs) lie deep within the largest gravitationally bound structures in existence. Though some cluster finding techniques identify the position of the BCG and use it as the cluster center, other techniques may not automatically ...
Patrick Janulewicz+2 more
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Utilizing Voronoi Tessellations to Determine Radial Density Profiles
We have developed a novel method of determining 2D radial density profiles for astronomical systems of discrete objects using Voronoi tessellations. This Voronoi-based method was tested against the standard annulus-based method on five simulated systems ...
Veronika Dornan, William E. Harris
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