Analysis of the Internal Radial Gradient of Chemical Abundances in Spiral Galaxies from CALIFA
The study of chemical evolution is of paramount importance for understanding the evolution of galaxies. Models and observations propose an inside-out mechanism in the formation of spiral galaxy disks, implying a negative radial gradient of elemental ...
A. F. S. Cardoso +3 more
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Investigating the Origins of Spiral Structure in Disk Galaxies through a Multiwavelength Study [PDF]
Ryan Miller +7 more
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THE LARSON-TINSLEY EFFECT IN THE ULTRAVIOLET: INTERACTING VERSUS “NORMAL” SPIRAL GALAXIES [PDF]
Beverly J. Smith, Curtis Struck
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Galaxy Zoo: 3D – crowdsourced bar, spiral, and foreground star masks for MaNGA target galaxies [PDF]
Karen L. Masters +17 more
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Living with Neighbors. V. Better-aligned Spiral+Spiral Galaxy Pairs Show Stronger Star Formation
Enhanced star formation (SF) with star-forming neighboring galaxies bolsters the hydrodynamical contributions during paired interactions. Although the relative spin orientation between interacting galaxies can influence this effect, it has not been ...
Woong-Bae G. Zee +3 more
doaj +1 more source
"Fermi" bubbles are bursting from our galaxy. Their origins remain a mystery. [PDF]
Mann A.
europepmc +1 more source
Mapping the Active Galactic Nucleus Effects on the Stellar and Gas Properties of NGC 5806
It is commonly accepted that active galactic nuclei (AGNs) have a strong impact upon the evolution of their host galaxies, but the processes by which they do so are not fully understood.
Sophie L. Robbins +2 more
doaj +1 more source
Magnetic fields in the nearby spiral galaxy IC 342: A multi-frequency radio polarization study [PDF]
R. Beck
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Internal kinematics of spiral galaxies in distant clusters [PDF]
Elif Kutdemir +10 more
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Ordered and chaotic spirals in disk galaxies [PDF]
P. A. Patsis +1 more
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