Modeling the Milky Way disk dynamics
Modeling the Milky Way disk dynamics
Modeling the Milky Way disk dynamics
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Groups and resonances (Monari et al, in prep.)BAR model20 o Ωp=49 km/s/kpcORBITALFREQUENCIESbar reference frameωR (=κ)ωϕ (=|Ω-Ωp|)Fourier transformωϕ (km/s/kpc)ωR (km/s/kpc)ωR/ωϕT. Antoja Sydney, 24/07/2012