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pro vyhledávání: '"Kang, Young Woon"'
Autor:
Jeong, Ji Young, Park, Jeong Ah, Kim, Jae Sung, Choi, Ji Yeon, Kang, Young Woon, Hwang, In Min
Publikováno v:
Analytical Letters; 2024, Vol. 57 Issue 16, p2585-2597, 13p
Autor:
Kang, Young Woon
This research was conducted to assess the feasibility of turkey processing wastewater treatment with a sand filter system. The effects of operational parameters such as hydraulic and organic loadings, filter design, dosing frequency, and detergent as
Externí odkaz:
http://rave.ohiolink.edu/etdc/view?acc_num=osu1078903968
Akademický článek
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Autor:
Lee, Jae-Woo, Lopez-Morales, Mercedes, Hong, Kyeong-Soo, Kang, Young-Woon, Pohl, Brian L., Walker, Alistair
We present BV photometry for 54 variables in the metal-rich inner halo globular cluster NGC6723. With the discovery of new RR Lyrae variables (RRLs), we obtain = 0.541 +/- 0.066 and = 0.292 +/- 0.030 day, n(c)/n(ab+c) = 0.167, and
Externí odkaz:
http://arxiv.org/abs/1311.2054
The most massive globular cluster in the Milky Way, omega Centauri, is thought to be the remaining core of a disrupted dwarf galaxy, as expected within the model of hierarchical merging. It contains several stellar populations having different heavy
Externí odkaz:
http://arxiv.org/abs/0911.4798
Autor:
Yushchenko, Alexander, Gopka, Vera, Goriely, Stephane, Shavrina, Angelina, Kang, Young Woon, Rostopchin, Sergey, Valyavin, Gennady, Mkrtichian, David, Hatzes, Artie, Lee, Byeong-Cheol, Kim, Chulhee
The abundance anomalies in chemically peculiar B-F stars are usually explained by diffusion of chemical elements in the stable atmospheres of these stars. But it is well known that Cp stars with similar temperatures and gravities show very different
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610611
Autor:
Yushchenko, Alexander, Gopka, Vera, Goriely, Stephane, Musaev, Faig, Shavrina, Angelina, Kim, Chulhee, Kang, Young Woon, Kuznietsova, Juliana, Yushchenko, Vladimir
We report the abundance determination in the atmosphere of the bright halo star HD221170. The spectra were taken with the Terskol Observatory's 2.0-m telescope with a resolution R=45000 and signal-to-noise ratio up to 250 in the wavelength region 363
Externí odkaz:
http://arxiv.org/abs/astro-ph/0409547
Publikováno v:
Astrophys.J.598:553-559,2003
We present a spectrum of the symbiotic star V1016 Cyg observed with the 3.6 m Canada-France-Hawaii Telescope, in order to illustrate a method to measure the covering factor of the neutral scattering region around the giant component with respect to t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0308084
Autor:
Han, Cheongho, Kang, Young Woon
Publikováno v:
Astrophys.J. 596 (2003) 1320-1326
Under the current microlensing planet search strategy of monitoring events caused by stellar-mass lenses, only planets located within a narrow region of separations from central stars can be effectively detected. However, with the dramatic increase o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0303317
Publikováno v:
CNU-PHYS-12/2001
If a gravitational microlensing event is caused by a widely separated binary lens and the source approaches both lens components, the source flux is successively magnified by the individual lenses: double microlensing events. If events are observed a
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112124