The Galactic warp revealed by Gaia DR2 kinematics
@article{Poggio2018TheGW, title={The Galactic warp revealed by Gaia DR2 kinematics}, author={Eloisa Poggio and Ronald Drimmel and Mario Gilberto Lattanzi and Richard L. Smart and Alessandro Spagna and Ren{\'e} Andrae and Coryn A. L. Bailer-Jones and Morgan Fouesneau and T. Antoja and C. Babusiaux and D. W. Evans and Francesca Figueras and David Katz and C'eline Reyl'e and Annie C. Robin and Manuel Romero‐Gomez and George Seabroke}, journal={Monthly Notices of the Royal Astronomical Society: Letters}, year={2018} }
Using Gaia DR2 astrometry, we map the kinematic signature of the Galactic stellar warp out to a distance of 7 kpc from the Sun. Combining Gaia DR2 and 2MASS photometry, we identify, via a probabilistic approach, 599 494 upper main sequence stars and 12 616 068 giants without the need for individual extinction estimates. The spatial distribution of the upper main sequence stars clearly shows segments of the nearest spiral arms. The large-scale kinematics of both the upper main sequence and giant…
61 Citations
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43 References
The kinematic signature of the Galactic warp in Gaia DR1 - I. The Hipparcos subsample
- Physics
- 2017
The mechanism responsible for the warp of our Galaxy, as well as its dynamical nature, continues to remain unknown. With the advent of high precision astrometry, new horizons have been opened for…
Characterizing the Galactic warp with Gaia - I. The tilted ring model with a twist
- Physics
- 2014
We explore the possibility of detecting and characterizing the warp of the stellar disc of our Galaxy using synthetic Gaia data. The availability of proper motions and, for the brightest stars radial…
Radial distribution of stellar motions in Gaia DR2
- Physics, GeologyMonthly Notices of the Royal Astronomical Society: Letters
- 2018
By taking advantage of the superb measurements of position and velocity for an unprecedented large number of stars provided in Gaia DR2, we have generated the first maps of the rotation velocity,…
Warp, waves, and wrinkles in the Milky Way
- Physics
- 2017
We derive unbiased distance estimates for the Gaia-TGAS data set by correcting for the bias due to the distance dependence of the selection function, which we measure directly from the data. From…
Unexpected stellar velocity distribution in the warped Galactic disk
- PhysicsNature
- 1998
It is now over 40 years since radio observations of neutral hydrogen revealed the gaseous disk of our Galaxy to be warped. Subsequently, the warp has been detected in the distribution of Galactic…
TRIGONOMETRIC PARALLAXES OF HIGH MASS STAR FORMING REGIONS: THE STRUCTURE AND KINEMATICS OF THE MILKY WAY
- Physics
- 2014
Over 100 trigonometric parallaxes and proper motions for masers associated with young, high-mass stars have been measured with the Bar and Spiral Structure Legacy Survey, a Very Long Baseline Array…
The Galactic warp as seen from 2MASS survey
- Physics
- 2008
The 2MASS survey is used to trace the shape of the external Galaxy where an asymmetric warp is detected. We use the Besancon Galaxy model to quantify the parameters of the stellar warp in the outer…
Vertical velocities from proper motions of red clump giants
- Physics
- 2014
Aims. We derive the vertical velocities of disk stars in the range of Galactocentric radii of R = 5−16 kpc within 2 kpc in height from the Galactic plane. This kinematic information is connected to…
Gaia Data Release 2
- Physics, GeologyAstronomy & Astrophysics
- 2018
Context. The second Gaia data release (Gaia DR2) contains high-precision positions, parallaxes, and proper motions for 1.3 billion sources as well as line-of-sight velocities for 7.2 million stars…
Galactic disc warps due to intergalactic accretion flows onto the disc
- Physics, Geology
- 2002
The accretion of the intergalactic medium onto the gaseous disc is used to explain the generation of galactic warps. A cup-shaped distortion is expected, due to the transmission of the linear…