output
19932026
Showing 2016 · astro-ph.GAShow all

27 papers · 2 filters

astro-ph.GA2016★ 4 cited

Early Science with the Large Millimeter Telescope: discovery of the 12CO(1-0) emission line in the ring galaxy, VIIZw466

O. Ivy Wong, O. Vega, D. Sánchez-Argüelles +9

We report an early science discovery of the CO(1-0) emission line in the collisional ring galaxy, VII Zw466, using the Redshift Search Receiver instrument on the Large Millimeter T…

astro-ph.GA2016★ 163 cited

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…

astro-ph.GA2016★ 15 cited

Discovery of five low luminosity active galactic nuclei at the centre of the Perseus cluster

Songyoun Park, Jun Yang, J. B. Raymond Oonk +1

According to optical stellar kinematics observations, an over-massive black hole candidate has been reported by van den Bosch et al. (2012) in the normal early-type galaxy NGC 1277…

astro-ph.GA2016★ 34 cited

THE NEXT GENERATION VIRGO CLUSTER SURVEY. XIV. Shell feature early-type dwarf galaxies in the Virgo cluster

Sanjaya Paudel, Rory Smith, Pierre-Alain Duc +15

The Next Generation Virgo Cluster Survey is a deep (with a detection limit = 29~mag~arcsec in the band) optical panchromatic survey targeting the Virgo cluste…

astro-ph.GA2016★ 22 cited

Common Origin of Two RR Lyrae Populations and the Double Red Clump in the Milky Way Bulge

Young-Wook Lee, Sohee Jang

A recent survey toward the Milky Way bulge has discovered two sequences of RR Lyrae stars on the period-amplitude diagram with a maximum period-shift of Δlog P = 0.015 between the…

astro-ph.GA2016★ 58 cited

Large-scale filamentary structures around the Virgo cluster revisited

Suk Kim, Soo-Chang Rey, Martin Bureau +9

We revisit the filamentary structures of galaxies around the Virgo cluster, exploiting a larger dataset based on the HyperLeda database than previous studies. In particular, this i…

astro-ph.GA2016★ 108 cited

The Preferential Tidal Stripping of Dark Matter versus Stars in Galaxies

Rory Smith, Hoseung Choi, Jaehyun Lee +3

Using high resolution hydrodynamical cosmological simulations, we conduct a comprehensive study of how tidal stripping removes dark matter and stars from galaxies. We find that dar…

astro-ph.GA2016★ 23 cited

Reversed radial distribution trend of subpopulations in the globular clusters NGC 362 and NGC 6723

Dongwook Lim, Young-Wook Lee, Mario Pasquato +2

Most globular clusters (GCs) are now known to host multiple stellar populations with different light element abundances. Here we use narrow-band photometry and low-resolution spect…

astro-ph.GA2016★ 49 cited

Unravelling the complex structure of AGN-driven outflows: II. Photoionization and energetics

Marios Karouzos, Jong-Hak Woo, Hyun-Jin Bae

Outflows have been shown to be prevalent in galaxies hosting luminous active galactic nuclei (AGNs) and present a physically plausible way to couple the AGN energy output with the…

astro-ph.GA2016★ 23 cited

The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119

Sree Oh, Sukyoung K. Yi, Luca Cortese +25

Galaxy mergers are important events that can determine the fate of a galaxy by changing its morphology, star-formation activity and mass growth. Merger systems have commonly been i…

astro-ph.GA2016★ 30 cited

New insight on the origin of the double red clump in the Milky Way bulge

Seok-Joo Joo, Young-Wook Lee, Chul Chung

The double red clump (RC) observed in the Milky Way bulge is widely interpreted as evidence for an X-shaped structure. We have recently suggested, however, an alternative interpret…

astro-ph.GA2016★ 41 cited

Abundance ratios and IMF slope in the dwarf elliptical galaxy NGC~1396 with MUSE

J. J. Mentz, F La Barbera, R. F. Peletier +16

Deep observations of the dwarf elliptical (dE) galaxy NGC 1396 (M, Mass M), located in the Fornax cluster, have been performed with the VLT/…

astro-ph.GA2016★ 11 cited

Could Segue 1 be a destroyed star cluster? - a dynamical perspective

Raul Dominguez, Michael Fellhauer, Matias Blaña +5

We attempt to find a progenitor for the ultra-faint object Segue 1 under the assumption that it formed as a dark matter free star cluster in the past. We look for orbits, using the…

astro-ph.GA2016★ 16 cited

Attack of the Flying Snakes : Formation of Isolated HI Clouds By Fragmentation of Long Streams

R. Taylor, J. I. Davies, P. Jachym +5

The existence of long (> 100 kpc) HI streams and small (< 20 kpc) free-floating HI clouds is well-known. While the formation of the streams has been investigated extensively, and t…

astro-ph.GA2016★ 22 cited

Recent galaxy mergers and residual star formation of red sequence galaxies in galaxy clusters

Yun-Kyeong Sheen, Sukyoung K. Yi, Chang H. Ree +3

This study explored the GALEX ultraviolet (UV) properties of optical red sequence galaxies in 4 rich Abell clusters at z \leq 0.1. In particular, we tried to find a hint of merger-…

astro-ph.GA2016★ 84 cited

The Prevalence of Gas Outflows in Type 2 AGNs. II. 3D Biconical Outflow Models

Hyun-Jin Bae, Jong-Hak Woo

We present 3D models of biconical outflows combined with a thin dust plane for investigating the physical properties of the ionized gas outflows and their effect on the observed ga…

astro-ph.GA2016★ 110 cited

BUDHIES III: The fate of HI and the quenching of galaxies in evolving environments

Yara L. Jaffé, Marc A. W. Verheijen, Chris P. Haines +13

In a hierarchical Universe clusters grow via the accretion of galaxies from the field, groups and even other clusters. As this happens, galaxies can lose their gas reservoirs via d…

astro-ph.GA2016★ 120 cited

Highest Redshift Image of Neutral Hydrogen in Emission: A CHILES Detection of a Starbursting Galaxy at z=0.376

Ximena Fernández, Hansung B. Gim, J. H. van Gorkom +32

Our current understanding of galaxy evolution still has many uncertainties associated with the details of accretion, processing, and removal of gas across cosmic time. The next gen…

astro-ph.GA2016★ 32 cited

The Demographics of galactic bulges in the SDSS database

Keunho Kim, Sree Oh, Hyunjin Jeong +3

We present a new database of our two-dimensional bulge-disk decompositions for 14,233 galaxies drawn from SDSS DR12 in order to examine the properties of bulges residing in the loc…

astro-ph.GA2016★ 10 cited

Globular clusters hosting intermediate-mass black-holes: no mass-segregation based candidates

Mario Pasquato, Paolo Miocchi, Bong Won Sohn +1

Recently, both stellar mass-segregation and binary-fractions were uniformly measured on relatively large samples of Galactic Globular Clusters (GCs). Simulations show that both siz…

astro-ph.GA2016★ 44 cited

Timing the evolution of quiescent and star-forming local galaxies

Camilla Pacifici, Sree Oh, Kyuseok Oh +2

Constraining the star formation histories (SFHs) of individual galaxies is crucial to understanding the mechanisms that regulate their evolution. Here, we combine multi-wavelength…

astro-ph.GA2016★ 33 cited

The Globular Cluster System of the Coma cD Galaxy NGC 4874 from Hubble Space Telescope ACS and WFC3/IR Imaging

Hyejeon Cho, John P. Blakeslee, Ana L. Chies-Santos +4

We present new HST optical and near-infrared (NIR) photometry of the rich globular cluster (GC) system of NGC 4874, the cD galaxy in the core of the Coma cluster (Abell 1656). NGC…

astro-ph.GA2016★ 87 cited

Local Volume TiNy Titans: Gaseous Dwarf-Dwarf Interactions in the Local Universe

Sarah Pearson, Gurtina Besla, Mary E. Putman +8

In this paper, we introduce the Local Volume TiNy Titans sample (LV-TNT), which is a part of a larger body of work on interacting dwarf galaxies: TNT (Stierwalt et al. 2015). This…

astro-ph.GA2016★ 14 cited

Galaxy Luminosity Function of Dynamically Young Abell 119 Cluster: Probing the Cluster Assembly

Youngdae Lee, Soo-Chang Rey, Michael Hilker +2

We present the galaxy luminosity function (LF) of the Abell 119 cluster down to mag based on deep images in the -, -, and -bands taken by using MOSAIC II CCD…