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- W172242274 abstract "For the purpose of this Paper, I will define the central region of the galaxy as being the inner four kiloparsecs. I make this definition for three reasons: 1) Outside of four kiloparsecs, the rotation curve for the galaxy is well-defined by the Schmidt disk model; whereas, inside four kiloparsecs, the effects of a central spherical component on the rotation curve become conspicuous. This inner spheroid is a dynamical component of the galaxy which is distinct from the disk and may be distinct from the extended halo component as well. 2) There is a conspicuous hole in the total gas density distribution inside 4 kpc. 3) High peculiar or non-circular gas velocities are observed within the inner 4 kpc; velocities ranging from the 53 km s -1 of the so-called 3 kpc arm, to 165 km s -1 in the molecular clouds within 300 pc of the center. I will now discuss these points in some greater detail." @default.
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- W172242274 date "1977-09-01" @default.
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- W172242274 title "Dynamical Effects in the Central Region of the Galaxy" @default.
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- W172242274 doi "https://doi.org/10.1017/s0252921100067403" @default.
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