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Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
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33 papers · 2 filters
Dust properties in the cold and hot gas phases of the ATLAS3D early-type galaxies as revealed by AKARI
T. Kokusho, H. Kaneda, M. Bureau +6
The properties of the dust in the cold and hot gas phases of early-type galaxies (ETGs) are key to understand ETG evolution. We thus conducted a systematic study of the dust in a l…
Nonlinear Color-Metallicity Relations of Globular Clusters. VIII. Reproducing Color Distributions of Individual Globular Cluster Systems in the Virgo and Fornax Galaxy Clusters
Sang-Yoon Lee, Chul Chung, Suk-Jin Yoon
The color distributions of globular clusters (GCs) in individual early-type galaxies show great diversity in their morphology. Based on the conventional "linear" relationship betwe…
The Fornax Deep Survey with VST. V. Exploring the faintest regions of the bright early-type galaxies inside the virial radius
E. Iodice, M. Spavone, M. Capaccioli +15
This paper is based on the multi-band (ugri) Fornax Deep Survey (FDS) with the VLT Survey Telescope (VST). We study bright early-type galaxies (m_B<15 mag) in the 9 square degrees…
CHILES: HI morphology and galaxy environment at z=0.12 and z=0.17
Kelley M. Hess, Nicholas M. Luber, Ximena Fernández +27
We present a study of 16 HI-detected galaxies found in 178 hours of observations from Epoch 1 of the COSMOS HI Large Extragalactic Survey (CHILES). We focus on two redshift ranges…
The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups
A. L. Schaefer, S. M. Croom, N. Scott +25
We explore the radial distribution of star formation in galaxies in the SAMI Galaxy Survey as a function of their local group environment. Using a sample of galaxies in groups (wit…
Theoretical Predictions of Colors and Metallicity of the Intra-Cluster Light
E. Contini, S. K. Yi, X. Kang
We study colors and metallicities of the Brightest Cluster Galaxies (BCGs) and Intra-Cluster Light (ICL) in galaxy groups and clusters, as predicted by a semi-analytic model of gal…
The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last 10 Gyr
Alfred L. Tiley, A. M. Swinbank, C. M. Harrison +16
We analyse maps of the spatially-resolved nebular emission of 1500 star-forming galaxies at - from deep KMOS and MUSE observations to measure the average…
Blue Straggler Bimodality: a Brownian Motion Model
Mario Pasquato, Paolo Miocchi, Suk-Jin Yoon
The shape of the radial distribution of Blue Straggler Stars (BSS), when normalized to a reference population of Horizontal Branch (HB) stars, has been found to be a powerful indic…
The Effect of Galaxy Interactions on Molecular Gas Properties
Hsi-An Pan, Lihwai Lin, Bau-Ching Hsieh +26
Galaxy interactions are often accompanied by an enhanced star formation rate (SFR). Since molecular gas is essential for star formation, it is vital to establish whether, and by ho…
The ALMA Detection of Extraplanar 13CO in a Ram-pressure-stripped Galaxy and Its Implication
Bumhyun Lee, Aeree Chung
NGC 4522 is a Virgo spiral that is currently undergoing active ram pressure stripping. In previous single-dish observations, 12CO emission was detected outside of the stellar disk,…
JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: I. Survey overview and first results
Amelie Saintonge, Christine D. Wilson, Ting Xiao +88
JINGLE is a new JCMT legacy survey designed to systematically study the cold interstellar medium of galaxies in the local Universe. As part of the survey we perform 850um continuum…
YZiCS: Preprocessing of dark halos in the hydrodynamic zoom-in simulation of clusters
San Han, Rory Smith, Hoseung Choi +4
To understand the galaxy population in clusters today, we should also consider the impact of previous environments prior to cluster infall, namely preprocessing. We use YZiCS, a hy…
On the origin of gas-poor galaxies in galaxy clusters using cosmological hydrodynamic simulations
Seoyoung L. Jung, Hoseung Choi, O. Ivy Wong +3
The environmental effect is commonly used to explain the excess of gas-poor galaxies in galaxy clusters. Meanwhile, the presence of gas-poor galaxies at cluster outskirts, where ga…
KUG 0200-096: Dwarf antennae hosting a tidal dwarf galaxy
Sanjaya Paudel, Chandreyee Sengupta, Suk Jin Yoon
We study a gas rich merging dwarf system KUG 0200-096. Deep optical image reveals an optically faint tail with a length of 20 kpc, giving a visual impression of tidal antenna simil…
Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
Rachel Asquith, Frazer R. Pearce, Omar Almaini +24
We present a comparison of the observed evolving galaxy stellar mass functions with the predictions of eight semi-analytic models and one halo occupation distribution model. While…
Wobbling galaxy spin axes in dense environments
Jaehyun Lee, Suk Kim, Hyunjin Jeong +7
The orientation of galaxy spin vectors within the large scale structure has been considered an important test of our understanding of structure formation. We investigate the angula…
A catalog of merging dwarf galaxies in the local universe
Sanjaya Paudel, Rory Smith, Suk Jin Yoo +2
We present the largest publicly available catalog of interacting dwarf galaxies. It includes 177 nearby merging dwarf galaxies of stellar mass M 10M$_{\sun}$ and r…
The different growth pathways of Brightest Cluster Galaxies and the Intra-Cluster Light
E. Contini, S. K. Yi, X. Kang
We study the growth pathways of Brightest Central Galaxies (BCGs) and Intra-Cluster Light (ICL) by means of a semi-analytic model. We assume that the ICL forms by stellar stripping…
Explaining the multiple populations in globular clusters by multiple episodes of star formation and enrichment without gas expulsion from massive star feedback
Jenny J. Kim, Young-Wook Lee
In order to investigate the origin of multiple stellar populations found in globular clusters (GCs) in the halo and bulge of the Milky Way, we have constructed chemical evolution m…
Assembling the Milky Way bulge from globular clusters: Evidence from the double red clump
Young-Wook Lee, Seungsoo Hong, Dongwook Lim +4
The two red clumps (RCs) observed in the color-magnitude diagram of the Milky Way bulge is widely accepted as evidence for an X-shaped structure originated from the bar instability…
KYDISC: Galaxy Morphology, Quenching, and Mergers in the Cluster Environment
Sree Oh, Keunho Kim, Joon Hyeop Lee +8
We present the KASI-Yonsei Deep Imaging Survey of Clusters (KYDISC) targeting 14 clusters at 0.015 < z < 0.144 using the Inamori Magellan Areal Camera and Spectrograph on the 6.5-m…
Galactic HCO+ Absorption toward Compact Extragalactic Radio Sources
Geumsook Park, Bon-Chul Koo, Kee-Tae Kim +2
As part of the search for the "dark molecular gas (DMG)," we report on the results of HCO J = 1-0 absorption observations toward nine bright extragalactic millimeter wave conti…
Evidence for the existence of abundant intracluster light at z= 1.24
Jongwan Ko, M. James Jee
Intracluster stars are believed to be unbound from their progenitor galaxies and diffused throughout the galaxy cluster, creating intracluster light (ICL). However, when and how th…
The MALATANG Survey: the L_gas-L_IR correlation on sub-kiloparsec scale in six nearby star-forming galaxies as traced by HCN J=4-3 and HCO^+ J=4-3
Qing-Hua Tan, Yu Gao, Zhi-Yu Zhang +43
We present HCN J=4-3 and HCO^+ J=4-3 maps of six nearby star-forming galaxies, NGC 253, NGC 1068, IC 342, M82, M83, and NGC 6946, obtained with the James Clerk Maxwell Telescope as…