THE ASYMMETRIC DRIFT AND THE ROTATION CURVE OF THE GALAXY
Asymmetric drift in the solar neighbourhood is studied by the means of the RAVE data. The asymmetric drift correction is applied to the SDSS data to measure the rotation curve of the Milky Way in the extended solar neighbourhood. The rotation curve is flat between7 and 10 kpc. Via fitting this flat...
Main Author: | O. Golubov |
---|---|
Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2014-10-01
|
Series: | Odessa Astronomical Publications |
Subjects: | |
Online Access: | http://oap.onu.edu.ua/article/view/80783 |
Similar Items
-
Gas Accretion Can Drive Turbulence in Galaxies
by: John C. Forbes, et al.
Published: (2023-01-01) -
Effects of the Central Mass Concentration on Bar Formation in Disk Galaxies
by: Dajeong Jang, et al.
Published: (2023-01-01) -
PROBES. I. A Compendium of Deep Rotation Curves and Matched Multiband Photometry
by: Connor Stone, et al.
Published: (2022-01-01) -
Probing the History of the Galaxy Assembly of the Counterrotating Disk Galaxy PGC 66551
by: Ivan Yu. Katkov, et al.
Published: (2024-01-01) -
On the Decline of Star Formation during the Evolution of Galaxies
by: Adelheid Teklu, et al.
Published: (2023-01-01)