22k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Massachusetts Institute of TechnologyUS255 papers
- California Institute of TechnologyUS233 papers
- Triangle Universities Nuclear LaboratoryUS232 papers
- Center for Astrophysics Harvard & SmithsonianUS218 papers
- Duke UniversityUS195 papers
- University of California, BerkeleyUS186 papers
- Lawrence Berkeley National LaboratoryUS185 papers
- Centre National de la Recherche ScientifiqueFR182 papers
- University of WashingtonUS182 papers
- Princeton UniversityUS178 papers
- The University of Texas at AustinUS168 papers
- Vanderbilt UniversityUS159 papers
12 papers · 2 filters
The SAMI Galaxy Survey: Revisiting Galaxy Classification Through High-Order Stellar Kinematics
Jesse van de Sande, Joss Bland-Hawthorn, Lisa M. R. Fogarty +36
Recent cosmological hydrodynamical simulations suggest that integral field spectroscopy can connect the high-order stellar kinematic moments h3 (~skewness) and h4 (~kurtosis) in ga…
DUSTiNGS III: Distribution of Intermediate-Age and Old Stellar Populations in Disks and Outer Extremities of Dwarf Galaxies
Kristen B. W. McQuinn, Martha L. Boyer, Mallory B. Mitchell +8
We have traced the spatial distributions of intermediate-age and old stars in nine dwarf galaxies in the distant parts of the Local Group, using multi-epoch 3.6 and 4.5 micron data…
The impact of magnetic fields on the chemical evolution of the supernova-driven ISM
Anabele-Linda Pardi, Philipp Girichidis, Thorsten Naab +7
We present three-dimensional magneto-hydrodynamical simulations of the self-gravitating interstellar medium (ISM) in a periodic (256 pc) box with a mean number density of 0.5 c…
The RESOLVE Survey Atomic Gas Census and Environmental Influences on Galaxy Gas Reservoirs
David V. Stark, Sheila J. Kannappan, Kathleen D. Eckert +17
We present the HI mass inventory for the RESOLVE survey, a volume-limited, multi-wavelength census of >1500 z=0 galaxies spanning diverse environments and complete in baryonic mass…
The SAMI Galaxy Survey: Asymmetry in Gas Kinematics and its links to Stellar Mass and Star Formation
J. V. Bloom, L. M. R. Fogarty, S. M. Croom +23
We study the properties of kinematically disturbed galaxies in the SAMI Galaxy Survey using a quantitative criterion, based on kinemetry (Krajnovic et al.). The approach, similar t…
Incidence of WISE-Selected Obscured AGNs in Major Mergers and Interactions from the SDSS
Madalyn E. Weston, Daniel H. McIntosh, Mark Brodwin +4
We use the Wide-field Infrared Survey Explorer (WISE) and the Sloan Digital Sky Survey (SDSS) to confirm a connection between dust-obscured active galactic nuclei (AGNs) and galaxy…
Reorienting MHD Colliding Flows: A Shock Physics Mechanism for Generating Filaments Normal to Magnetic Fields
Erica L. Fogerty, Jonathan Carroll-Nellenback, Adam Frank +2
We present numerical simulations of reorienting oblique shocks that form in the collision layer between magnetized colliding flows. Reorientation aligns parsec-scale post-shock fil…
Chemical enrichment of the pre-solar cloud by supernova dust grains
Matthew D. Goodson, Ian Luebbers, Fabian Heitsch +1
The presence of short-lived radioisotopes (SLRs) in solar system meteorites has been interpreted as evidence that the solar system was exposed to a supernova shortly before or duri…
Scaling Relations of Starburst-Driven Galactic Winds
Ryan Tanner, Gerald Cecil, Fabian Heitsch
Using synthetic absorption lines generated from 3D hydro-dynamical simulations we explore how the velocity of a starburst-driven galactic wind correlates with the star formation ra…
Three-Dimensional Orientation of Compact High Velocity Clouds
F. Heitsch, B. Bartell, S. E. Clark +3
We present a proof-of-concept study of a method to estimate the inclination angle of compact high velocity clouds (CHVCs), i.e. the angle between a CHVC's trajectory and the line-o…
RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
Kathleen D. Eckert, Sheila J. Kannappan, David V. Stark +3
In this work, we present galaxy stellar and baryonic (stars plus cold gas) mass functions (SMF and BMF) and their halo mass dependence for two volume-limited data sets. The first,…
Molecular cloud formation in high-shear, magnetized colliding flows
Erica Fogerty, Adam Frank, Fabian Heitsch +3
The colliding flows (CF) model is a well-supported mechanism for generating molecular clouds. However, to-date most CF simulations have focused on the formation of clouds in the no…