Results 61 to 70 of about 1,738 (137)
Retarded Gravity in Disk Galaxies
Disk galaxies have a typical dimension of a few tens of kiloparsecs. It follows from the theory of general relativity that any signal originating from the galactic center will be noticed at the outskirts of the galaxy only tens of thousands of years later.
Yuval Glass +2 more
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AbstractWe review our knowledge about the spiral structure of the disk of our Galaxy using tracers of star formation. These tracers reveal a 4-arm picture of the Galaxy.
openaire +1 more source
We calculate the stellar surface mass density (Sigma_*) and two-component (gas+stars) disk stability (Q_RW) for 25 late-type galaxies from the DiskMass Survey. These calculations are based on fits of a dynamical model to our ionized-gas and stellar kinematic data performed using a Markov Chain Monte Carlo sampling of the Bayesian posterior ...
Westfall, K. B. +5 more
openaire +4 more sources
Counter-Rotation in Disk Galaxies
Counter-rotating galaxies host two components rotating in opposite directions with respect to each other. The kinematic and morphological properties of lenticulars and spirals hosting counter-rotating components are reviewed. Statistics of the counter-rotating galaxies and analysis of their stellar populations provide constraints on the formation ...
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ON THE SPIRAL STRUCTURE OF DISK GALAXIES
C. C. Lin, Frank H. Shu
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A direct black-hole mass measurement in a little red dot at high redshift. [PDF]
Juodžbalis I +39 more
europepmc +1 more source
Evidence for a sub-Jovian planet in the young TWA 7 disk. [PDF]
Lagrange AM +28 more
europepmc +1 more source
A giant disk galaxy two billion years after the Big Bang. [PDF]
Wang W +16 more
europepmc +1 more source
Accurate determination of chemical abundances near a supermassive black hole. [PDF]
XRISM Collaboration.
europepmc +1 more source
Discovery of a high-velocity cloud of the Milky Way as a potential dark galaxy. [PDF]
Liu XL +8 more
europepmc +1 more source

