C II forbidden-line 158 micron mapping in Sagittarius A Rotation curve and mass distribution in the galactic center

Astronomy and Astrophysics – Astronomy

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Carbon, Galactic Nuclei, Galactic Rotation, Infrared Astronomy, Mass Distribution, Milky Way Galaxy, Astronomical Maps, Maximum Entropy Method, Rotating Disks

Scientific paper

The authors have mapped the 158 μm fine structure line emission of C+ over a region of ≡30 pc diameter toward the galactic center. They use the kinematic information from the C+ profiles together with a computer model of a turbulent, rotating disk to derive the rotation curve and mass distribution between 2 and 10 pc from the center. The measurements are well fitted by a thin, azimuthally symmetric disk of inclination ≡65° in Keplerian rotation around a central point mass of 6.5±1×106M_sun;. The best overall mass model, including all presently available data, indicates 5 - 6×106M_sun; within 2 pc from IRS 16 and 8 - 15×106M_sun; within 10 pc of IRS 16. The mass to luminosity ratio of the central stellar cluster is 0.5 M_sun;/L_sun; or less, suggesting a large abundance of giants and relatively recent star formation in the center.

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