Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Y. C. Minh"'
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 22, Iss 2, Pp 125-138 (2005)
S152 is a small bright emission nebula located in the Perseus arm. Its optical diameter corresponds to 1.5 pc for an adopted distance 3.5 kpc. However, S152 is a part of a giant molecular cloud complex, which consists of several dense cores, containi
Externí odkaz:
https://doaj.org/article/91425220b6394b848be76fdaed381512
Autor:
Y. C. Minh
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 21, Iss 4, Pp 233-242 (2004)
The HCO^+ 1--0 transition line was observed toward the Sgr B2 region in our Galactic center. We found that there exist two large-scale velocity structures of vlsr ˜50 and ˜100 km/s, which are thought to interact with each other. A new gas clump ``O
Externí odkaz:
https://doaj.org/article/47714c5f1d954b0389979e89978d23ff
Autor:
Rene P. Breton, Dhota Pradipta, Y. C. Minh, Taufiq Hidayat, L. Puspitarini, H. R. T. Wulandari, P. Jaroenjittichai, Sébastien Lambert, Mohammad Hafieduddin, Koichiro Sugiyama, Kenta Fujisawa, Dudy D. Wijaya, N. Liu, Tomoya Hirota, Ibnu Nurul Huda, Sahlan Ramadhan, Premana Premadi, Nabila S. E. Putri, Stephane Leon, Budi Dermawan, Yoshinori Yonekura
Publikováno v:
Experimental Astronomy. 52:141-155
In the near future, two radio telescopes will be installed in the Indonesian region. These telescopes are proposed to be integrated into the existing Very Long Baseline Interferometry (VLBI) network both for astronomical and geodetical purposes. Here
Autor:
G. S. Orton, Steve Miller, Sang Joon Kim, Thomas R. Geballe, Y. C. Minh, Yuk L. Yung, Thomas K. Greathouse
Publikováno v:
Icarus. 281:281-285
We have derived homopause temperatures of 180–250 K for the 8-µm north-polar hot spot (8NPHS) of Jupiter by fitting CH_4 emission models to 3 and 8 µm spectra of the 8NPHS obtained 24 days apart in 2013. From the fits, we find that CH_4 mixing ra
Publikováno v:
Publications of The Korean Astronomical Society. 31:57-63
Publikováno v:
The Astrophysical Journal. 723:1231-1240
The massive star-forming core MM1 of W75N was observed using the Submillimeter Array with {approx}1'' and 2'' spatial resolutions at 217 and 347 GHz, respectively. From the 217 GHz continuum we found that the MM1 core consists of two sources, separat
Publikováno v:
The Astrophysical Journal. 720:1-8
We observed the Sh 2-233IR (S233IR) region with better sensitivity in near-infrared than previous studies for this region. By applying statistical subtraction of the back- ground stars, we identified member sources and derived the age and mass of thr
Publikováno v:
The Astrophysical Journal. 697:428-435
We report the synthesis of glycine on interstellar ice-analog films composed of water, methylamine (MA), and carbon dioxide under irradiation of ultraviolet (UV) photons. Analysis of the UV-irradiated ice films by in situ mass spectrometric methods r
Autor:
Christopher J. Davis, Sang-Gak Lee, Soojong Pak, Y C Minh, Minho Choi, Thomas R. Geballe, Sungho Lee, Paul T. P. Ho, Robeson M. Herrnstein
Publikováno v:
Journal of Physics: Conference Series. 54:22-28
We have surveyed the interaction regions between Sgr A East and the surrounding molecular clouds in the H2 1-0 S(l) (2.1218 μm) line emission. The resulting data cube shows the distribution of the H2 emission both in space (with a resolution of abou
Autor:
John H. Black, B. Rowe, William M. Irvine, Karl M. Menten, Alexander Dalgarno, Carsten Henkel, Y. C. Minh, John P. Maier, L. E. Snyder, P. D. Singh, E. F. van Dishoeck, V. Buch, J. M. Greenberg, D.A. Williams, L.W. Avery, M. Ohishi, Q. Zeng
Publikováno v:
Transactions of the International Astronomical Union. 24:281-284
The field of Molecular Astrophysics or “Astrochemistry” has grown considerably since its inception in the late 1930’s. Molecules have been observed in astronomical environments as diverse as comets in the solar system and galaxies at the highes