Results 61 to 70 of about 1,814 (135)
The Formation of Disk Galaxies [PDF]
In this talk, I will discuss a few particular topics, rather than attempting a general review of the formation of disk galaxies. First recall the basic structure and kinematics of a disk galaxy like the Milky Way. The Table below lists the four main structural components as they are presently understood, and gives typical masses, and (if known) the ...
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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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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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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
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Star formation powers optical line emission from the CGM. [PDF]
Zhang H +11 more
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Overmassive black holes and little red dots naturally form in simulations. [PDF]
Chon S +4 more
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Introducing GalaxyR: an easy-to-use R implementation of the Galaxy API. [PDF]
Frey J +12 more
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A Discrete Informational Framework for Classical Gravity: Ledger Foundations and Galaxy Rotation Curve Constraints. [PDF]
Simons M, Allahyarov E, Washburn J.
europepmc +1 more source
The orbital dynamics of the LMC and SMC about the Milky Way. [PDF]
Besla G, Kallivayalil N.
europepmc +1 more source
ON THE SPIRAL STRUCTURE OF DISK GALAXIES
C. C. Lin, Frank H. Shu
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