output
20072026
most citedSuppression of magnetic ordering in XXZ-type antiferromagnetic monolayer NiPS3

455 citations

Showing 2014 · astro-ph.GAShow all

12 papers · 2 filters

astro-ph.GA2014★ 62 cited

Cosmic Evolution of Black Holes and Spheroids. V. The Relation Between Black Hole Mass and Host Galaxy Luminosity for a Sample of 79 Active Galaxies

Daeseong Park, Jong-Hak Woo, Vardha N. Bennert +3

We investigate the cosmic evolution of the black hole (BH) mass -- bulge luminosity relation using a sample of 52 active galaxies at and in the BH mass…

astro-ph.GA2014★ 8 cited

Instability of Magnetized Ionization Fronts Surrounding H II Regions

Jeong-Gyu Kim, Woong-Tae Kim

An ionization front (IF) surrounding an H II region is a sharp interface where a cold neutral gas makes transition to a warm ionized phase by absorbing UV photons from central star…

astro-ph.GA2014★ 13 cited

Discovery of an Ultra-Faint Dwarf Galaxy in the Intracluster Field of the Virgo Center : A fossil of the First Galaxies?

In Sung Jang, Myung Gyoon Lee

Ultra-faint dwarf galaxies (UFDs) are newcomers among galaxies, and are the faintest galaxies in the observed universe. To date, they have only been found around the Milky Way Gala…

astro-ph.GA2014★ 75 cited

A Census of Gas Outflows in Type 2 Active Galactic Nuclei

Hyun-Jin Bae, Jong-Hak Woo

We perform a census of ionized gas outflows using a sample of ~23,000 type 2 active galactic nuclei (AGNs) out to z~0.1. By measuring the velocity offset of narrow emission lines,…

astro-ph.GA2014★ 28 cited

The Tip of the Red Giant Branch Distance to the Perfect Spiral Galaxy M74 Hosting Three Core-Collapse Supernovae

In Sung Jang, Myung Gyoon Lee

M74 (NGC 628) is a famous face-on spiral galaxy, hosting three core-collapse supernovae (SNe):SN Ic 2002ap, SN II-P 2003gd, and SN II-P 2013ej. However its distance is not well kno…

astro-ph.GA2014★ 20 cited

Effects of Spiral Arms on Star Formation in Nuclear Rings of Barred-spiral Galaxies

Woo-Young Seo, Woong-Tae Kim

We use hydrodynamic simulations to study the effect of spiral arms on the star formation rate (SFR) occurring in nuclear rings of barred-spiral galaxies. We find that spiral arms c…

astro-ph.GA2014★ 14 cited

Alignments of the Galaxies in and around the Virgo Cluster with the Local Velocity Shear

Jounghun Lee, Soo-Chang Rey, Suk Kim

An observational evidence is presented for the alignment between the cosmic sheet and the principal axis of the velocity shear field at the position of the Virgo cluster. The galax…

astro-ph.GA2014★ 18 cited

The AGN Population in X-ray Selected Galaxy Groups at

Semyeong Oh, John S. Mulchaey, Jong-Hak Woo +6

We use Chandra data to study the incidence and properties of Active Galactic Nuclei (AGN) in 16 intermediate redshift () X-ray-selected galaxy groups in the Chandra…

astro-ph.GA2014★ 51 cited

Nature of the Wiggle Instability of Galactic Spiral Shocks

Woong-Tae Kim, Yonghwi Kim, Jeong-Gyu Kim

Gas in disk galaxies interacts nonlinearly with an underlying stellar spiral potential to form galactic spiral shocks. While numerical simulations typically show that spiral shocks…

astro-ph.GA2014★ 15 cited

Steadily Increasing Star Formation Rates in Galaxies Observed at 3 <~ z <~ 5 in the CANDELS/GOODS-S Field

Seong-Kook Lee, Henry C. Ferguson, Rachel S. Somerville +3

We investigate the star formation histories (SFHs) of high redshift (3 <~ z <~ 5) star-forming galaxies selected based on their rest-frame ultraviolet (UV) colors in the CANDELS/GO…

astro-ph.GA2014★ 58 cited

Three Dimensional Hydrodynamic Simulations of Multiphase Galactic Disks with Star Formation Feedback: II. Synthetic HI 21 cm Line Observations

Chang-Goo Kim, Eve C. Ostriker, Woong-Tae Kim

We use three-dimensional numerical hydrodynamic simulations of the turbulent, multiphase atomic interstellar medium (ISM) to construct and analyze synthetic HI 21 cm emission and a…

astro-ph.GA2014★ 56 cited

A New Optical Survey of Supernova Remnant Candidates in M31

Jong Hwan Lee, Myung Gyoon Lee

We present a survey of optically emitting supernova remnants (SNRs) in M31 based on H and [SII] images in the Local Group Survey. Using these images, we select objects that have…