Dynamical Properties of Galactic OH/IR Stars
نویسندگان
چکیده
منابع مشابه
Dynamical Evolution of the Young Stars in the Galactic Center: N-body Simulations of the S-stars
We use N -body simulations to study the evolution of the orbital eccentricities of stars deposited near (. 0.05 pc) the Milky Way massive black hole (MBH), starting from initial conditions motivated by two competing models for their origin: formation in a disk followed by inward migration; and exchange interactions involving a binary star. The first model predicts modest eccentricities, lower t...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1996
ISSN: 0074-1809
DOI: 10.1017/s0074180900229902