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UNBIASED WATER AND METHANOL MASER SURVEYS OF NGC 1333
Lyo, A-Ran,Kim, Jongsoo,Byun, Do-Young,Lee, Ho-Gyu American Institute of Physics 2014 The Astronomical journal Vol.148 No.5
<P>We present the results of unbiased 22 GHz H<SUB>2</SUB>O water and 44 GHz class I CH<SUB>3</SUB>OH methanol maser surveys in the central 7' × 10' area of NGC 1333 and two additional mapping observations of a 22 GHz water maser in a ~3' × 3' area of the IRAS4A region. In the 22 GHz water maser survey of NGC 1333 with a sensitivity of σ ~ 0.3 Jy, we confirmed the detection of masers toward H<SUB>2</SUB>O(B) in the region of HH 7-11 and IRAS4B. We also detected new water masers located ~20'' away in the western direction of IRAS4B or ~25'' away in the southern direction of IRAS4A. We could not, however, find young stellar objects or molecular outflows associated with them. They showed two different velocity components of ~0 and ~16 km s<SUP>–1</SUP>, which are blue- and redshifted relative to the adopted systemic velocity of ~7 km s<SUP>–1</SUP> for NGC 1333. They also showed time variabilities in both intensity and velocity from multi-epoch observations and an anti-correlation between the intensities of the blue- and redshifted velocity components. We suggest that the unidentified power source of these masers might be found in the earliest evolutionary stage of star formation, before the onset of molecular outflows. Finding this kind of water maser is only possible through an unbiased blind survey. In the 44 GHz methanol maser survey with a sensitivity of σ ~ 0.5 Jy, we confirmed masers toward IRAS4A2 and the eastern shock region of IRAS2A. Both sources are also detected in 95 and 132 GHz methanol maser lines. In addition, we had new detections of methanol masers at 95 and 132 GHz toward IRAS4B. In terms of the isotropic luminosity, we detected methanol maser sources brighter than ~5 × 10<SUP>25</SUP> erg s<SUP>–1</SUP> from our unbiased survey.</P>
THE LONGEVITY OF CIRCUMSTELLAR DISKS: THE η CHAMAELEONTIS CLUSTER
LYO A-RAN,LAWSON W. A. The Korean Astronomical Society 2005 Journal of The Korean Astronomical Society Vol.38 No.2
We have analysed near-infrared JHKL observations of the members of the $\approx$9 Myr-old $\eta$ Chamaeleontis cluster. Using (J - H)/(K - L) and (H - K)/(K - L) IR colour-colour diagrams for the brightest 15 members of the cluster, we find the fraction of stellar systems with near-IR excess emission was 0.60 $\pm$ 0.13 (2$\sigma$). For the CTT and WTT star population, we also find a strong correlation between the IR excess and Ha emission which is also known as an accretion indicator. The (K - L) excess of these stars appears to indicate a wide range of star-disk activity; from a CTT star with high levels of accretion, to CTT - WTT transitional objects with evidence for some on-going accretion, and WTT stars with weak or absent IR excesses. Among the brightest 15 members, four stars (RECX 5, 9, 11 and ECHA J0843.3-7905) with IR excesses ${\Delta}$(K - L) > 0.4 mag and strong or variable optical emission were identified as likely experiencing on-going mass accretion from their circumstellar disks which we confirmed their accretion disks from the optical high-resolution echelle spectroscopic study. The result-ing accretion fraction of 0.27 $\pm$ 0.13 (2$\sigma$) suggests that the accretion phase, in addition to the disks themselves, can endure for at least ${\~}$10 Myr.
Intraventricular and Subarachnoid Fat after Spinal Injury
Lyo, In-Uk,Sim, Hong-Bo,Park, Jun-Bum,Kwon, Soon-Chan The Korean Neurosurgical Society 2008 Journal of Korean neurosurgical society Vol.44 No.2
The authors report an extremely rare case with intraventricular and subarachnoid fat developed after trauma to spine and soft tissue in a 54-year-old male. The initial computed tomography (CT) showed multiple low attenuation lesions, which were thought to be pneumocephalus. Cerebral magnetic resonance imaging (MRI) showed lesions with high signal intensity on T1-weighted magnetic resonance images and high signal intensity on T2-weighted images, indicating fat globules within the CSF. In this report, the clinical presentation, radiological findings, and a review of the literature are presented.
Inner Warm Disk of ESO H<i>α</i>279a Revealed by NA i and CO Overtone Emission Lines
Lyo, A-Ran,Kim, Jongsoo,Lee, Jae-Joon,Kim, Kyoung-Hee,Kang, Jihyun,Byun, Do-Young,Mace, Gregory,Sokal, Kimberly R.,Park, Chan,Chun, Moo-Young,Oh, Heeyoung,Yu, Young Sam,Oh, Jae Sok,Jeong, Ueejeong,Kim American Astronomical Society 2017 The Astrophysical Journal Vol.844 No.1
<P>We present an analysis of near-infrared, high-resolution spectroscopy toward the flat-spectrum young stellar object (YSO) ESO H alpha 279a (similar to 1.5M(circle dot)) in the Serpens star-forming region at a distance of 429 pc. Using the Immersion GRating INfrared Spectrometer (IGRINS; R approximate to 45,000), we detect emission lines originating from the accretion channel flow, jet, and inner disk. Specifically, we identify hydrogen Brackett series recombination, [Fe II], [Fe III], [Fe IV], Ca I, Na I, H-2, H2O, and CO overtone emission lines. By modeling five bands of CO overtone emission lines and the symmetric double-peaked line profile for Na I emission lines, we find that ESO H alpha 279a has an actively accreting Keplerian disk. From our Keplerian disk model, we find that Na I emission lines originate between 0.04 and 1.00 au, while the CO overtone emission lines are from the outer part of the disk, in the range between 0.22 and 3.00 au. The model reveals that the neutral atomic Na gas is a good tracer of the innermost region of the actively accreting disk. We derive a mass accretion rate of 2-10 x 10-7 Me yr(-1). from the measured Br gamma emission luminosity of 1.78(+/- 0.31) x 10(31) erg s(-1).</P>
Transverse Fracture and Dislocation at the Sacrum
Lyo, In-Uk,Kwon, Soon-Chan,Park, Jun-Bum,Sim, Hong-Bo The Korean Neurosurgical Society 2008 Journal of Korean neurosurgical society Vol.43 No.1
We present a rare case of fracture-dislocation at the level of the first sacral (S1) and second sacral (S2) vertebrae. The S1 was displaced forward into the pelvic cavity and was located just in front of the S2. Because the patient also had extensive neurological injury to the lumbar plexus and instability of the pelvic ring, surgery to stabilize the pelvis and to decompress the lumbar plexus was performed. The surgery was successful and the patient experienced marked improvement in neurological function.
Lyo Min Kwon,Myungsu Lee 소화기인터벤션의학회 2020 Gastrointestinal Intervention Vol.9 No.3
Benign afferent loop obstruction (ALO) is a complication that occurs after general surgery making Roux-en-Y or Billroth-II reconstruction and has typically been treated surgically. However, the surgery is difficult to conduct in about 25% of cases due to comorbidity and nonoperative management has been attempted. Here, we report two cases of benign ALO that were treated with percutaneous transhepatic afferent loop balloon dilatation and indwelling catheter, including one case with no improvement after surgery.
Lyo Min Kwon,Myungsu Lee 소화기인터벤션의학회 2020 International journal of gastrointestinal interven Vol.9 No.3
Benign afferent loop obstruction (ALO) is a complication that occurs after general surgery making Roux-en-Y or Billroth-II reconstruction and has typically been treated surgically. However, the surgery is difficult to conduct in about 25% of cases due to comorbidity and nonoperative management has been attempted. Here, we report two cases of benign ALO that were treated with percutaneous transhepatic afferent loop balloon dilatation and indwelling catheter, including one case with no improvement after surgery.