Results 1 to 10 of about 7,775 (165)
A Milky Way-like barred spiral galaxy at a redshift of 3. [PDF]
Costantin L+32 more
europepmc +3 more sources
We show the variations of the CO J = 2–1/1–0 line ratio ( R _21/10 ) across the barred spiral galaxy M83, using the 46 pc resolution data from the Atacama Large Millimeter/submillimeter Array. The R _21/10 map clearly evidences the systematic large-scale
Jin Koda+5 more
doaj +2 more sources
Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions [PDF]
Famaey B, McGaugh SS.
exaly +2 more sources
On the plausible origins of the spiral character of galaxies
We here-in demonstrate that the proposed hitherto unknown gravitomagnetic dark-force that hypothetically explains the Flat Rotation Curves of Spiral Galaxies — this same force, explains very well, the logarithmic and as-well, the barred spiral shapes of ...
Nyambuya Golden Gadzirayi
doaj +1 more source
AGN spiral galaxies in groups: effects of bars [PDF]
We explore properties of barred active spiral galaxies in groups selected from the SDSS-DR7, with the aim of assessing the effects of bars on AGN and the role of the high density environment.
Alonso, Sol+2 more
core +4 more sources
Formation of Major Types of Galaxies Based on the Energy Circulation Theory
The standard cosmology can answer almost nothing about how the structure of a galaxy is formed. It expects a supermassive black hole at the center and dark matter in the halo to explain the circulation of stars and its velocity.
Shigeto Nagao
doaj +1 more source
JWST/Mid-Infrared Instrument imaging of the nearby galaxies IC 5332, NGC 628, NGC 1365, and NGC 7496 from PHANGS reveals a richness of gas structures that in each case form a quasi-regular network of interconnected filaments, shells, and voids.
Sharon E. Meidt+33 more
doaj +1 more source
Large-scale bars can fuel galaxy centers with molecular gas, often leading to the development of dense ringlike structures where intense star formation occurs, forming a very different environment compared to galactic disks.
Eva Schinnerer+39 more
doaj +1 more source
We analyze TYPHOON long-slit-absorption line spectra of the starburst barred spiral galaxy NGC 1365 obtained with the Progressive Integral Step Method covering an area of 15 kpc ^2 .
Eva Sextl+8 more
doaj +1 more source
Mechanisms based on chaotic flows that support structures in barred-spiral systems
I summarize the dynamical mechanisms that have been found to shape structures such as the spirals and the bars in barred-spiral systems. Response models and orbital analysis are used to study the dynamics in potentials estimated from near-infrared images
Patsis P.A.
doaj +1 more source