Zobrazeno 1 - 10
of 14 275
pro vyhledávání: '"Sung, Chul"'
Autor:
Iwata, Yuhei, Akimoto, Masanori, Matsuoka, Tomoki, Maeda, Keiichi, Yonekura, Yoshinori, Tominaga, Nozomu, Moriya, Takashi J., Fujisawa, Kenta, Niinuma, Kotaro, Yoon, Sung-Chul, Lee, Jae-Joon, Jung, Taehyun, Byun, Do-Young
We report on radio follow-up observations of the nearby Type II supernova, SN 2023ixf, spanning from 1.7 to 269.9 days after the explosion, conducted using three very long baseline interferometers (VLBIs), which are the Japanese VLBI Network (JVN), t
Externí odkaz:
http://arxiv.org/abs/2411.07542
Publikováno v:
Nuclear Engineering and Technology, Vol 56, Iss 12, Pp 5022-5027 (2024)
The cross-sections of natTi(p,x) reactions were measured up to 50 MeV by using off-line γ-ray spectrometry and stacked-foil activation technique. The activation experiment was conducted using 57 MeV proton beams from the proton accelerator at the Ko
Externí odkaz:
https://doaj.org/article/3db02eb53a6f4b14adb4d12f28bc7633
Autor:
Ju Ri Ye, Seung Hwan Park, Sang Wook Kang, Kyu Hwan Kwack, Yong Kwon Chae, Hyo-Seol Lee, Sung Chul Choi, Ok Hyung Nam
Publikováno v:
BMC Oral Health, Vol 24, Iss 1, Pp 1-8 (2024)
Abstract Background Oxyresveratrol is the main constituent of mulberries and has many bioactive properties beneficial to human health. The purpose of this study was to assess the anti-inflammatory effects of oxyresveratrol on in vitro periodontitis m
Externí odkaz:
https://doaj.org/article/a88d2828b3424fb2b2e0599b536c8107
Previous numerical simulations of double-peaked SNe IIb light curves have demonstrated that the radius and mass of the hydrogen-rich envelope of the progenitor star can significantly influence the brightness and timescale of the early-time light curv
Externí odkaz:
http://arxiv.org/abs/2310.16328
Recent multi-media data such as images and videos have been rapidly spread out on various online services such as social network services (SNS). With the explosive growth of online media services, the number of image content that may harm users is al
Externí odkaz:
http://arxiv.org/abs/2310.05192
The Cassiopeia A supernova remnant has a complex structure, manifesting the multidimensional nature of core-collapse supernova explosions. To further understand this, we carried out near-infrared multi-object spectroscopy on the ejecta knots located
Externí odkaz:
http://arxiv.org/abs/2305.04484
Publikováno v:
Research in Plant Disease, Vol 30, Iss 3, Pp 256-267 (2024)
We have developed FBcastS (Fire Blight Forecasting System), a cloud-based information system that leverages the K-Maryblyt forecasting model. The FBcastS provides an optimal timing for spraying antibiotics to prevent flower infection caused by Erwini
Externí odkaz:
https://doaj.org/article/f492c8b6768c427a8b9d2397d05b5eb6
Type Ib and Ic supernovae (SNe Ib/Ic) originate from hydrogen-deficient massive star progenitors, of which the exact properties are still much debated. Using the SN data in the literature, we investigate the optical $B-V$ color of SNe Ib/Ic at the $V
Externí odkaz:
http://arxiv.org/abs/2304.10670
Publikováno v:
2023, The Astrophysical Journal, Volume 945, Issue 2, id.158
We report on the result of He abundance analysis of dense circumstellar clumps in the young supernova remnant Cassiopeia A. These clumps, which are called quasi-stationary flocculi (QSFs), are known from previous optical studies to be enriched in He
Externí odkaz:
http://arxiv.org/abs/2303.16497