Showing 2015 · astro-ph.GAShow all

48 papers · 2 filters

astro-ph.GA2015★ 13 cited

Evidence of Fanning in the Ophiuchus Stream

B. Sesar, A. M. Price-Whelan, J. G. Cohen +11

The Ophiuchus stellar stream presents a dynamical puzzle: its old stellar populations ( Gyr) cannot be reconciled with (1) its orbit in a simple model for the Milky Way po…

astro-ph.GA2015★ 2 cited

The Sizes of Globular Clusters as Tracers of Galactic Halo Potentials

Akram Hasani Zonoozi, Malihe Rabiee, Hosein Haghi +1

We present -body simulations of globular clusters, exploring the effect of different galactic potentials on cluster sizes, . For various galactocentric distances, , we…

astro-ph.GA2015★ 70 cited

Matching dust emission structures and magnetic field in high-latitude cloud L1642: comparing Herschel and Planck maps

J. Malinen, L. Montier, J. Montillaud +7

The nearby cloud L1642 is one of only two known very high latitude (|b| > 30 deg) clouds actively forming stars. It is a rare example of star formation in isolated conditions, and…

astro-ph.GA2015★ 98 cited

Role of Cosmic Rays in the Circumgalactic Medium

Munier Salem, Greg L. Bryan, Lauren Corlies

We explore the impact of cosmic rays (CRs) on cosmological adaptive-mesh refinement simulations of a forming 10^12 Msolar halo, focusing on the circumgalactic medium (CGM), and its…

astro-ph.GA2015

AGN feedback and star formation in ETGs: negative and positive feedback

L. Ciotti, J. P. Ostriker, A. Negri +3

AGN feedback from supermassive black holes (SMBHs) at the center of early type galaxies is commonly invoked as the explanation for the quenching of star formation in these systems.…

astro-ph.GA2015★ 478 cited

The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars

Vicente Rodriguez-Gomez, Annalisa Pillepich, Laura V. Sales +9

We use the Illustris simulation to study the relative contributions of in situ star formation and stellar accretion to the build-up of galaxies over an unprecedentedly wide range o…

astro-ph.GA2015★ 41 cited

Early Science with the Large Millimeter Telescope: COOL BUDHIES I - a pilot study of molecular and atomic gas at z~0.2

Ryan Cybulski, Min S. Yun, Neal Erickson +20

An understanding of the mass build-up in galaxies over time necessitates tracing the evolution of cold gas (molecular and atomic) in galaxies. To that end, we have conducted a pilo…

astro-ph.GA2015★ 46 cited

First Results from COPSS: The CO Power Spectrum Survey

Garrett K. Keating, Geoffrey C. Bower, Daniel P. Marrone +11

We present constraints on the abundance of carbon-monoxide in the early Universe from the CO Power Spectrum Survey (COPSS). We utilize a data set collected between 2005 and 2008 us…

astro-ph.GA2015★ 9 cited

A Statistical Method to Search for Recoiling Supermassive Black Holes in Active Galactic Nuclei

Peter Raffai, Zoltan Haiman, Zsolt Frei

We propose an observational test for gravitationally recoiling supermassive black holes (BHs) in active galactic nuclei, based on a correlation between the velocities of BHs relati…

astro-ph.GA2015

A NuSTAR Survey of Nearby Ultraluminous Infrared Galaxies

Stacy H. Teng, Jane R. Rigby, Daniel Stern +17

We present a NuSTAR, Chandra, and XMM--Newton survey of nine of the nearest ultraluminous infrared galaxies (ULIRGs). The unprecedented sensitivity of NuSTAR at energies above 10 k…

astro-ph.GA2015★ 45 cited

Evidence for the Thermal Sunyaev-Zel'dovich Effect Associated with Quasar Feedback

Devin Crichton, Megan B. Gralla, Kirsten Hall +20

Using a radio-quiet subsample of the Sloan Digital Sky Survey spectroscopic quasar catalogue, spanning redshifts 0.5-3.5, we derive the mean millimetre and far-infrared quasar spec…

astro-ph.GA2015

Globular Cluster Streams as Galactic High-Precision Scales

A. H. W. Küpper, E. Balbinot, A. Bonaca +4

Tidal streams of globular clusters are ideal tracers of the Galactic gravitational potential. Compared to the few known, complex and diffuse dwarf-galaxy streams, they are kinemati…

astro-ph.GA2015★ 99 cited

Tidal debris morphology and the orbits of satellite galaxies

David Hendel, Kathryn V. Johnston

How do galaxies move relative to one another? While we can examine the motion of dark matter subhalos around their hosts in simulations of structure formation, determining the orbi…

astro-ph.GA2015★ 59 cited

A Large Systematic Search for Close Supermassive Binary and Rapidly Recoiling Black Holes - II. Continued Spectroscopic Monitoring and Optical Flux Variability

Jessie C. Runnoe, Michael Eracleous, Gavin Mathes +6

We present new spectroscopic observations that are part of our continuing monitoring campaign of 88 quasars at z<0.7 whose broad H lines are offset from their systemic redshifts…

astro-ph.GA2015★ 71 cited

The NANOGrav Nine-year Data Set: Astrometric Measurements of 37 Millisecond Pulsars

Allison M. Matthews, David J. Nice, Emmanuel Fonseca +18

Using the nine-year radio-pulsar timing data set from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav), collected at Arecibo Observatory and the Green Ba…

astro-ph.GA2015★ 204 cited

Launching cosmic-ray-driven outflows from the magnetized interstellar medium

Philipp Girichidis, Thorsten Naab, Stefanie Walch +10

We present a hydrodynamical simulation of the turbulent, magnetized, supernova (SN)-driven interstellar medium (ISM) in a stratified box that dynamically couples the injection and…

astro-ph.GA2015★ 20 cited

Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines

Andrew Emerick, Greg Bryan, Mary E. Putman

Understanding gas flows into and out of the most massive dark matter structures in our Universe, galaxy clusters, is fundamental to understanding their evolution. Gas in clusters i…

astro-ph.GA2015★ 303 cited

Young Stellar Objects in the Gould Belt

Michael M. Dunham, Lori E. Allen, Neal J. Evans +14

We present the full catalog of Young Stellar Objects (YSOs) identified in the 18 molecular clouds surveyed by the Spitzer Space Telescope "cores to disks" (c2d) and "Gould Belt" (G…

astro-ph.GA2015★ 321 cited

The NANOGrav Nine-year Data Set: Limits on the Isotropic Stochastic Gravitational Wave Background

Zaven Arzoumanian, Adam Brazier, Sarah Burke-Spolaor +45

We compute upper limits on the nanohertz-frequency isotropic stochastic gravitational wave background (GWB) using the 9-year data release from the North American Nanohertz Observat…

astro-ph.GA2015★ 50 cited

Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation

Aaron D. Bray, Annalisa Pillepich, Laura V. Sales +9

Comparisons between observational surveys and galaxy formation models find that the mass of dark matter haloes can largely explain galaxies' stellar mass. However, it remains uncer…

astro-ph.GA2015★ 25 cited

ECO and RESOLVE: Galaxy Disk Growth in Environmental Context

Amanda J. Moffett, Sheila J. Kannappan, Andreas A. Berlind +5

We study the relationships between galaxy environments and galaxy properties related to disk (re)growth, considering two highly complete samples that are approximately baryonic mas…

astro-ph.GA2015★ 33 cited

The properties and the formation mechanism of the stellar counter-rotating components in NGC 4191

Lodovico Coccato, Maximilian Fabricius, Lorenzo Morelli +7

We disentangle two counter-rotating stellar components in NGC 4191 and characterize their physical properties (kinematics, morphology, age, metallicity, and abundance ratio). We pe…

astro-ph.GA2015★ 146 cited

Ram Pressure Stripping of the Large Magellanic Cloud's Disk as a Probe of the Milky Way's Circumgalactic Medium

Munier Salem, Gurtina Besla, Greg Bryan +3

Recent observations have constrained the orbit and structure of the Large Magellanic Cloud (LMC), implying a well-constrained pericentric passage about the Milky Way (MW) ~ 50 Myr…

astro-ph.GA2015★ 79 cited

Chaotic Dispersal of Tidal Debris

Adrian M. Price-Whelan, Kathryn V. Johnston, Monica Valluri +3

Several long, dynamically cold stellar streams have been observed around the Milky Way Galaxy, presumably formed from the tidal disruption of globular clusters. In integrable poten…