Mass Transfer in 토토 승무패 Systems of a White Dwarf
관련링크
본문
"Many interesting astrophysical phenomena are known in 토토 승무패 systems containing
a white dwarf when the companion star loses some its mass. White dwarf 토토 승무패 systems are progenitors of Type Ia supernovae, which are important to probe the accelerated expansion of the universe. Outward transport of
angular momenta leads to the formation of an accretion disk around the white dwarf.
Many details in accretion flow are known in close 토토 승무패 systems, which are
collectively called cataclysmic variables. Much less is known in the case of
wide binaries known as symbiotic stars, where mass transfer is achieved via gravitational
capture of slow stellar wind. In this talk, a brief introdcution
to accretion phenomena in 토토 승무패 systems of a white dwarf will be given with
some observational results obtained from Mt. Bohyun.
"