The GALAH survey: velocity fluctuations in the Milky Way using Red Clump giants
Copyright policy )The GALAH survey: velocity fluctuations in the Milky Way using Red Clump giants
If the Galaxy is axisymmetric and in dynamical equilibrium, we expect negligible fluctuations in the residual line-of-sight velocity field. Recent results using the \apg{} survey find significant fluctuations in velocity for stars in the midplane ($|z|
20 pages, 16 figures, accepted for publication in MNRAS
- Australian National University Australia
- University of California, Berkeley United States
- Max Planck Society Germany
- Australian Astronomical Observatory Australia
- University of Sydney Australia
astrophysics, anzsrc-for: 5107 Particle and high energy physics, anzsrc-for: 5101 Astronomical Sciences, FOS: Physical sciences, 612, 530, Astrophysics - Astrophysics of Galaxies, 520, anzsrc-for: 0201 Astronomical and Space Sciences, 5101 Astronomical Sciences, Astrophysics of Galaxies (astro-ph.GA), galaxies, stars: distances, stars: fundamental parameters, anzsrc-for: 5109 Space sciences, anzsrc-for: 51 Physical Sciences, 51 Physical Sciences, Galaxy: kinematics and dynamics
astrophysics, anzsrc-for: 5107 Particle and high energy physics, anzsrc-for: 5101 Astronomical Sciences, FOS: Physical sciences, 612, 530, Astrophysics - Astrophysics of Galaxies, 520, anzsrc-for: 0201 Astronomical and Space Sciences, 5101 Astronomical Sciences, Astrophysics of Galaxies (astro-ph.GA), galaxies, stars: distances, stars: fundamental parameters, anzsrc-for: 5109 Space sciences, anzsrc-for: 51 Physical Sciences, 51 Physical Sciences, Galaxy: kinematics and dynamics
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