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Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. VI: An evidence for the long lived non-steady warp of non-gravitational scenarios
H. -F. Wang, M. López-Corredoira, Y. Huang +6
By combining LAMOST DR4 and Gaia DR2 common red clump stars with age and proper motion, we analyze the amplitude evolution of the stellar warp independently of any assumption with…
Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. II. 3D asymmetrical kinematics of mono-age populations in the disk between 6 \,kpc
H. -F. Wang, M. López-Corredoira, Y. Huang +11
We perform analysis of the three-dimensional kinematics of Milky Way disk stars in mono-age populations. We focus on stars between Galactocentric distances of and 14 \,kpc, s…
3D Asymmetrical motions of the Galactic outer disk with LAMOST K giant stars
Haifeng Wang, Martín López-Corredoira, Jeffrey L. Carlin +1
We present a three dimensional velocity analysis of Milky Way disk kinematics using LAMOST K giant stars and the GPS1 proper motion catalogue. We find that Galactic disk stars near…
Three-dimensional decomposition of galaxies with bulge and long bar
Paul Compère, Martín López-Corredoira, Francisco Garzón
Some observations indicate that the Milky Way has two inner components, a bulge and a long bar, which present a misalignment of about 20 degrees that is against the predictions of…
The long bar as seen by the VVV Survey: II. Star counts
Eduardo Amôres, Martín López-Corredoira, Carlos González-Fernández +3
Context: There is still some debate about the presence and the morphological properties of the long bar in the inner Galaxy. Aims: We investigate the morphological properties of th…
The long bar as seen by the VVV survey: I. Colour-magnitude diagrams
C. González-Fernández, M. López-Corredoira, E. B. Amôres +3
The VISTA Variable Survey (VVV) is able to map the Galaxy at l<0 with an unpaired depth (at least 3 mag deeper than 2MASS), opening new possibilities for studying the inner structu…