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...

Full description

Saved in:
Bibliographic Details
Published in:The Astrophysical journal 2012-11, Vol.759 (2), p.1-20
Main Authors: BOVY, Jo, ALLENDE PRIETO, Carlos, GIRARDI, Léo, HEARTY, Fred R, HOGG, David W, HOLTZMAN, Jon, MAIA, Marcio A. G, MAJEWSKI, Steven R, MALANUSHENKO, Elena, MALANUSHENKO, Viktor, MESZAROS, Szabolcs, NIDEVER, David L, BEERS, Timothy C, O'CONNELL, Robert W, O'DONNELL, Christine, ORAVETZ, Audrey, PAN, Kaike, ROCHA-PINTO, Helio J, SCHIAVON, Ricardo P, SCHNEIDER, Donald P, SCHULTHEIS, Mathias, SKRUTSKIE, Michael, SMITH, Verne V, BIZYAEV, Dmitry, WEINBERG, David H, WILSON, John C, ZASOWSKI, Gail, DA COSTA, Luiz N, CUNHA, Katia, EBELKE, Garrett L, ELSENSTEIN, Daniel J, FRINCHABO, Peter M, ELIA GARCIA PEREZ, Ana
Format: Article
Language:eng
Subjects:
SUN
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
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]).
ISSN:0004-637X
1538-4357