76 citations · 174 across the 26 of their papers we have counts for
26 papers
CHILES VI: HI and H Observations for z < 0.1 Galaxies; Probing HI Spin Alignment with Filaments in the Cosmic Web
J. Blue Bird, J. Davis, N. Luber +15
We present neutral hydrogen (HI) and ionized hydrogen (H) observations of ten galaxies out to a redshift of 0.1. The HI observations are from the first epoch (178 hours) of the…
Massive Compact Galaxies with High-Velocity Outflows: Morphological Analysis and Constraints on AGN Activity
P. H. Sell, C. A. Tremonti, R. C. Hickox +9
We investigate the process of rapid star formation quenching in a sample of 12 massive galaxies at intermediate redshift (z~0.6) that host high-velocity ionized gas outflows (v>100…
Cluster Galaxy Morphologies: The Relationship among Structural Parameters, Activity and the Environment
Christopher Añorve, Omar López-Cruz, Hector Ibarra-Medel +1
We use an approach to estimate galaxy morphologies based on an ellipticity (e) vs. Bulge-to-Total ratio (B/T) plane. We have calibrated this plane by comparing with Dressler's clas…
Cluster magnetic fields from active galactic nuclei
P. M. Sutter, P. M. Ricker, H. -Y. Yang
Active galactic nuclei (AGN) found at the centers of clusters of galaxies are a possible source for weak cluster-wide magnetic fields. To evaluate this scenario, we present 3D adap…
Calibrating AGN Feedback in Clusters
M. W. Wise
Whether caused by AGN jets, shocks, or mergers, the most definitive evidence for heating in cluster cores comes from X-ray spectroscopy. Unfortunately such spectra are essentially…
AGN Feedback: Does it work?
Smita Mathur, Rebecca Stoll, Yair Krongold +3
While feedback is important in theoretical models, we do not really know if it works in reality. Feedback from jets appears to be sufficient to keep the cooling flows in clusters f…