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of 45
pro vyhledávání: '"Young Chol Minh"'
Autor:
Young Chol Minh, Sang Joon Ki
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 28, Iss 1, Pp 13-16 (2011)
The CH3OH 4_2–5_1 E transition was observed toward the Sgr B2 region, including the Principal Cloud and its surroundings. This methanol transition shows an extended emission along the 2’N cloud, which is believed to be colliding with the Princi
Externí odkaz:
https://doaj.org/article/d345adc2c392400687a315ef8f56bf02
Akademický článek
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Autor:
Young Chol Minh, Paul T. P. Ho, Izaskun Jiménez-Serra, Qizhou Zhang, Roberto Galván-Madrid, Carlos Román-Zúñiga, Adam Ginsburg, Hauyu Baobab Liu, Huei-Ru Vivien Chen, Leonardo Testi
We report new, $\sim$1000 AU spatial resolution observations of 225 GHz dust continuum emission towards the OB cluster-forming molecular clump G33.92+0.11. On parsec scales, this molecular clump presents a morphology with several arm-like dense gas s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d37510bdbb1a03a6fc3bb58fb2c0c58
http://arxiv.org/abs/1808.07702
http://arxiv.org/abs/1808.07702
Publikováno v:
Publications of The Korean Astronomical Society. 30:133-137
The Galactic center uniquely provides opportunities to resolve how star clusters form in neutral gas overdensities engulfed in a large-scale accretion flow. We have performed sensitive Green Bank 100m Telescope (GBT), Karl G. Jansky Very Large Array
Autor:
X. Z. Zhang, Yong Sun Park, Young Chol Minh, Seokho Lee, Yi Jeng Kuan, Kee-Tae Kim, Chi-Hung Yan, Tatsuhiko I. Hasegawa, Dharam Vil Lal
Publikováno v:
Journal of The Korean Astronomical Society. 47:179-185
We study the physical and chemical properties of the molecular clump hosting a young stellar cluster, IRAS 20160+3636, which is believed to have formed via the “collect and collapse” process. Physical parameters of the UC Hii region associated wi
Autor:
Young Chol Minh
Publikováno v:
Publications of The Korean Astronomical Society. 29:29-34
Publikováno v:
Journal of The Korean Astronomical Society. 45:157-166
Using the Submillimeter Array (SMA), we identified two bright hot subcores, MM1a and MM1b (size ~ 1” and mass ~ 0.5 M ⊙ ) separated by about 1.6”, in the 230 ㎓ continuum emission toward the massive star-forming region DR21(OH). Both display t
Autor:
Moo-Young Chun, Young Chol Minh, Kang-Min Kim, Jae Sok Oh, Soojong Pak, Heeyoung Oh, Tae-Soo Pyo, Hye-In Lee, Daniel T. Jaffe, In-Soo Yuk, Ueejeong Jeong, Gregory N. Mace, Sungho Lee, Kyle F. Kaplan, Young Sam Yu, Michael D. Pavel, Narae Hwang, Byeong-Gon Park, Huynh Anh N. Le, Chan Park
We have analyzed the temperature, velocity and density of H2 gas in NGC 7023 with a high-resolution near-infrared spectrum of the northwestern filament of the reflection nebula. By observing NGC 7023 in the H and K bands at R ~ 45,000 with the Immers
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d8b4db09746ff06f47bd2ac3c2271fa
Autor:
Sang Joon Kim, Young Chol Minh
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 28, Iss 1, Pp 13-16 (2011)
The CH3OH 4_2–5_1 E transition was observed toward the Sgr B2 region, including the Principal Cloud and its surroundings. This methanol transition shows an extended emission along the 2’N cloud, which is believed to be colliding with the Principa
Autor:
Hauyu Baobab Liu, Young Chol Minh, Jinhua He, Tatsuhiko I. Hasegawa, Roberto Galván-Madrid, Dipen Sahu
Publikováno v:
The Astrophysical Journal. 864:102
The central region of the massive star-forming cloud G33.92+0.11 was investigated with the emission from the deuterated species HDCS and DCN observed at sub-arcsecond angular resolution (~07) using ALMA. HDCS shows a distributed emission throughout t