Results 31 to 40 of about 8,688,256 (155)
The Milky Way is moving faster than before– It is likely to clash with other galaxies. In two billion years. Someone will have to go through that.
Ernesto Priego
core +1 more source
Minimum-entropy Constraints on Galactic Potentials
A tracer sample in a gravitational potential, starting from a generic initial condition, phase-mixes toward a stationary state. This evolution is accompanied by an entropy increase, and the final state is characterized by a distribution function (DF ...
Leandro Beraldo e Silva +5 more
doaj +1 more source
Stellar abundances in clusters: High-resolution, multi-object spectroscopy of globular & open clusters in the Milky Way [PDF]
Talk on high-resolution, multi-object spectroscopy of globular & open clusters in the Milky ...
BRAGAGLIA, Angela
core
An Inward-moving and Asymmetric Velocity Wave Detected in LAMOST-Gaia
The phase space, as coded by kinematic parameters and chemical abundances, is crucial for understanding the formation of the Galactic disk. Using red giant stars from the Galactic thin disk with [Fe/H] > − 0.8 and low- α ratios identified in LAMOST-Gaia,
Yuqin Chen +5 more
doaj +1 more source
Icarus Revisited: An Ancient, Metal-poor Accreted Stellar Stream in the Disk of the Milky Way
The search for accreted satellites in the Galactic disk is a challenging task, to which Gaia plays a crucial role in synergy with ground-based spectroscopic surveys. In 2021, P. Re Fiorentin et al.
Paola Re Fiorentin +4 more
doaj +1 more source
We briefly describe TRILEGAL, a TRIdimensional modeL of thE GALaxy, and its more recent developments. Particularly relevant is the recent inclusion of a kinematical module to the code, and the present efforts to provide a more solid calibration of Milky ...
Barbieri, Mauro +8 more
core +1 more source
Dynamical Models of the Milky Way in Action Space with LAMOST DR8 and Gaia EDR3
This work explores dynamical models of the Milky Way (MW) by analyzing a sample of 86,109 K giant stars selected through cross-matching the LAMOST DR8 and Gaia EDR3 surveys. Our earlier torus models of Q. Wang et al.
Guang-Chen Sun +8 more
doaj +1 more source
AuriDESI: mock catalogues for the DESI Milky Way Survey [PDF]
The Dark Energy Spectroscopic Instrument Milky Way Survey (DESI MWS) will explore the assembly history of the Milky Way by characterizing remnants of ancient dwarf galaxy accretion events and improving constraints on the distribution of dark matter in ...
de la Macorra, Axel +75 more
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Under the assumption of a simple and time-invariant gravitational potential, many Galactic dynamics techniques infer the milky Way’s mass and dark matter distributions from stellar kinematic observations.
Danny Horta +7 more
doaj +1 more source
The Milky Way (MW) is a barred spiral galaxy shaped by tidal interactions with its satellites. The Large Magellanic Cloud (LMC) and the Sagittarius dwarf galaxy (Sgr) are the dominant influences at the present day. This paper presents a suite of four 10 ^
Ioana A. Stelea +2 more
doaj +1 more source

