57 citations · 177 across the 10 of their papers we have counts for
10 papers
MIRIS Paα Galactic Plane Survey. II. The Catalog of Paα Emission-line Sources
Il-Joong Kim, Jeonghyun Pyo, Kwang-Il Seon +3
Using data from the MIRIS Paα Galactic Plane Survey (MIPAPS), we present a Paα 1.87 um line image of the entire Galactic plane within the latitude range of -3° < b < +3°, revealing…
High-resolution Near-infrared Spectroscopy of Diffuse Sources around MWC 1080
Il-Joong Kim, Heeyoung Oh, Woong-Seob Jeong +3
To reveal the origins of diffuse H-alpha emissions observed around the Herbig star MWC 1080, we have performed a high-resolution near-infrared (NIR) spectroscopic observation using…
MIRIS Paα Galactic Plane Survey. I. Comparison with IPHAS Hα in l = 96°-116°
Il-Joong Kim, Jeonghyun Pyo, Woong-Seob Jeong +11
The Multipurpose InfraRed Imaging System (MIRIS) performed the MIRIS Paα Galactic Plane Survey (MIPAPS), which covers the entire Galactic plane within the latitude range of -3° < b…
MIRIS observation of near-infrared diffuse Galactic light
Y. Onishi, K. Sano, S. Matsuura +17
We report near-infrared (IR) observations of high Galactic latitude clouds to investigate diffuse Galactic light (DGL), which is starlight scattered by interstellar dust grains. Th…
Diffuse Extraplanar Dust in NGC 891
Kwang-Il Seon, Adolf N. Witt, Jong-Ho Shinn +1
We report the detection of vertically extended far-ultraviolet (FUV) and near-UV emissions in an edge-on spiral galaxy NGC 891, which we interpret as being due to dust-scattered st…
Global Far-Ultraviolet Properties of the Cygnus Loop
Il-Joong Kim, Kwang-Il Seon, Yeo-Myeong Lim +4
We present the C III λ977, O VI λλ1032, 1038 and N IV] λ1486 emission line maps of the Cygnus Loop, obtained with the newly processed data of Spectroscopy of Plasma Evolution from…
Comparison of the Diffuse Halpha and FUV Continuum Backgrounds: On the Origins of the Diffuse Halpha Background
Kwang-Il Seon, Adolf Witt, Il-Joong Kim +4
We compare the diffuse H map of our Galaxy with the FUV (1370-1710Å) continuum map. The H intensity correlates well with the FUV intensity. The H/FUV intensity ratio incre…
Far-ultraviolet Emission-line Morphologies of the Supernova Remnant G65.3+5.7
I. -J. Kim, K. -I. Seon, K. -W. Min +3
We present the first far-ultraviolet (FUV) emission-line morphologies of the whole region of the supernova remnant (SNR) G65.3+5.7 using the FIMS/SPEAR data. The morphologies of th…
Observation of the Far-ultraviolet Continuum Background with SPEAR/FIMS
K. -I. Seon, J. Edelstein, E. Korpela +6
We present the general properties of the far-ultraviolet (FUV; 1370-1720A) continuum background over most of the sky, obtained with the Spectroscopy of Plasma Evolution from Astrop…
Far-Ultraviolet Cooling Features of the Antlia Supernova Remnant
Jong-Ho Shinn, Kyoung Wook Min, Ravi Sankrit +7
We present far-ultraviolet observations of the Antlia supernova remnant obtained with Far-ultraviolet IMaging Spectrograph (FIMS, also called SPEAR). The strongest lines observed a…