The Age Distribution of Stellar Orbit Space Clumps
The orbit distribution of young stars in the Galactic disk is highly structured, from well-defined clusters to streams of stars that may be widely dispersed across the sky, but are compact in orbital action-angle space.
Verena Fürnkranz +3 more
doaj +1 more source
Using nearly 230,000 red clump stars selected from LAMOST and Gaia, we conduct a comprehensive analysis of the stellar age–velocity dispersion relations (AVRs) for various disk populations, within 5.0 ≤ R ≤ 15.0 kpc and ∣ Z ∣ ≤ 3.0 kpc.
Weixiang Sun +3 more
doaj +1 more source
A computational method to dissect colonization resistance of the gut microbiota against pathogens. [PDF]
Ke S +5 more
europepmc +1 more source
Gas Transfer between the Inner 3 kpc Disk and the Galactic Central Molecular Zone
We uncovered a more tilted molecular gas structure with highly negative velocities located near the dust lane. Our observations show that the approaching gas flows from the overshoot process are captured by the gravitational potential of the bar and then
Yang Su +12 more
doaj +1 more source
Revealing Gas Inflows Toward the Galactic Central Molecular Zone
We study the gas inflows toward the Galactic Central Molecular Zone (CMZ) based on the gas morphological and kinematic features from the Milky Way Imaging Scroll Painting in the region of l = 1.°2–19.°0 and ∣ b ∣ ≲ 3.°0.
Yang Su +9 more
doaj +1 more source
Milky Way potentials in cold dark matter and MOdified Newtonian Dynamics. Is the Large Magellanic Cloud on a bound orbit? [PDF]
Xufen Wu +4 more
openalex +1 more source
First constraints on Fuzzy Dark Matter from the dynamics of stellar streams in the Milky Way
N. C. Amorisco, Abraham Loeb
openalex +2 more sources
The photometry and kinematics studies of NGC 2509 derived from Gaia DR3. [PDF]
Ahmed NM, Tadross AL.
europepmc +1 more source
Pixelation of perovskite quantum wire thin films with 0.18-μm features and 63,500-ppi pixel density. [PDF]
Zhang Q +13 more
europepmc +1 more source
Cluster Ages to Reconstruct the Milky Way Assembly (CARMA) IV. Chrono-dynamics of seven old star clusters in the Large Magellanic Cloud and the peculiar origin of NGC 1841 [PDF]
F. Niederhofer +17 more
openalex +1 more source

