Thank you for visiting my web site.
I'm 4th year Ph.D student majoring in Astrophysics at Sejong University in South Korea.
My research interests are mass transfer and mass accretion processes in symbiotic stars.
I'm fascinated with symbiotic star, which is consisting of a mass losing cool giant, a hot white dwarf and circumstellar material.
Mass transfer in form of a slow stellar wind from giant toward white dwarf cause various intriguing astrophysical phenomena including formation of an accretion disk, jet launching, X-ray emission form boundary layer between accretion disk and WD/thermonuclear reaction from the surface of WD, polarization of lights, etc.
Their active nature and complexity is what first attracted me to way to being professional astronomer.
Symbiotic stars are suitable laboratory to testing important astrophysical questions, such as understanding fundamental physics behind type Ia supernovae or evolution toward bipolar nebulae.
I'm trying to figure out quoted problems in numerical points of view, especially Radiative transfer and Hydrodynamics.
In the near future, I'm (naively) planning to extend my research area to radiative hydrodynamics of related objects and protoplanetary system.
Again, thank you for visiting my personal site. I wish I could share some of my interests to you.
I'm 4th year Ph.D student majoring in Astrophysics at Sejong University in South Korea.
My research interests are mass transfer and mass accretion processes in symbiotic stars.
I'm fascinated with symbiotic star, which is consisting of a mass losing cool giant, a hot white dwarf and circumstellar material.
Mass transfer in form of a slow stellar wind from giant toward white dwarf cause various intriguing astrophysical phenomena including formation of an accretion disk, jet launching, X-ray emission form boundary layer between accretion disk and WD/thermonuclear reaction from the surface of WD, polarization of lights, etc.
Their active nature and complexity is what first attracted me to way to being professional astronomer.
Symbiotic stars are suitable laboratory to testing important astrophysical questions, such as understanding fundamental physics behind type Ia supernovae or evolution toward bipolar nebulae.
I'm trying to figure out quoted problems in numerical points of view, especially Radiative transfer and Hydrodynamics.
In the near future, I'm (naively) planning to extend my research area to radiative hydrodynamics of related objects and protoplanetary system.
Again, thank you for visiting my personal site. I wish I could share some of my interests to you.