Zobrazeno 1 - 10
of 75
pro vyhledávání: '"Baek, Chang Hyun"'
Publikováno v:
In Annals of Nuclear Energy 15 September 2024 205
Publikováno v:
In Radiation Physics and Chemistry May 2024 218
Publikováno v:
In Nuclear Engineering and Technology November 2022 54(11):4095-4101
Publikováno v:
In Energy Strategy Reviews January 2022 39
Publikováno v:
Nuclear Technology and Radiation Protection, Vol 37, Iss 3, Pp 253-257 (2022)
As a historic challenge for humans, Martian colonization has been initiated by nuclear energy. A moving nuclear power plant could be imaginable known as a nuclear reactor rover. The design of the nuclear reactor rover has been performed where the
Externí odkaz:
https://doaj.org/article/9b2bec54add34beabca690a05c1c1290
Publikováno v:
International Journal of Green Energy. 2024, Vol. 21 Issue 6, p1201-1209. 9p.
Publikováno v:
Astrophys.J.690:944-952,2009
High-resolution SiO observations of the NGC 1333 IRAS 4A star-forming region showed a highly collimated outflow with a substantial deflection. The deflection was suggested to be caused by the interactions of the outflow and a dense cloud core. To inv
Externí odkaz:
http://arxiv.org/abs/0806.1095
Publikováno v:
Astrophys.J. 682 (2008) 434-444
The unusual mushroom-shaped HI cloud, GW 123.4--1.5, is hundreds of parsecs in size but does not show any correlations to HI shells or chimney structures. To investigate the origin and velocity structure of GW 123.4--1.5, we perform three-dimensional
Externí odkaz:
http://arxiv.org/abs/0801.3186
Publikováno v:
Astrophys.J. 643 (2006) L83-L86
Thermal-gravitational instability (TGI) is studied in the protogalactic environment. We extend our previous work, where we found that dense clumps first form out of hot background gas by thermal instability and later a small fraction of them grow to
Externí odkaz:
http://arxiv.org/abs/astro-ph/0604536
Publikováno v:
Astrophys.J. 630 (2005) 689-704
We study thermal-gravitational instability in simplified models for protogalactic halos using three-dimensional hydrodynamic simulations. The simulations followed the evolution of gas with radiative cooling down to T = 10^4 K, background heating, and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506160