THE MILKY WAY'S CIRCULAR-VELOCITY CURVE BETWEEN 4 AND 14 kpc FROM APOGEE DATA
We measure the Milky Way's rotation curve over the Galactocentric range 4 kpc [lap] R [lap] 14 kpc from the first year of data from the Apache Point Observatory Galactic Evolution Experiment. We determine the local value of the circular velocity to be V sub(c)(R sub(0)) = 218+ or -6kms super(-1...
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Published in: | The Astrophysical journal 2012-11, Vol.759 (2), p.1-20 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | eng |
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Online Access: | Get full text |
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Summary: | We measure the Milky Way's rotation curve over the Galactocentric range 4 kpc [lap] R [lap] 14 kpc from the first year of data from the Apache Point Observatory Galactic Evolution Experiment. We determine the local value of the circular velocity to be V sub(c)(R sub(0)) = 218+ or -6kms super(-1) and find that the rotation curve is approximately flat with a local derivative between -3.0kms super(-1) kpc super(-1) and 0.4kms super(-1) kpc super(-1). We investigate various systematic uncertainties and find that these are limited to offsets at the percent level, ~2kms super(-1) in V sub(c). Marginalizing over all the systematics that we consider, we find that V sub(c)(R sub(0)) < 235kms super(-1) at >99 % confidence. We find an offset between the Sun's rotational velocity and the local circular velocity of 26 + or - 3kms super(-1), which is larger than the locally measured solar motion of 12kms super(-1). Combining our results with other data, we find that the Milky Way's dark-halo mass within the virial radius is ~8 x 10 super(11) M sub([middot in circle]). |
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ISSN: | 0004-637X 1538-4357 |