Results 11 to 20 of about 476,460 (296)

Chaotic spiral galaxies [PDF]

open access: yesCelestial Mechanics and Dynamical Astronomy, 2011
We study the role of asymptotic curves in supporting the spiral structure of a N-body model simulating a barred spiral galaxy. Chaotic orbits with initial conditions on the unstable asymptotic curves of the main unstable periodic orbits follow the shape of the periodic orbits for an initial interval of time and then they are diffused outwards ...
M. Harsoula, George Contopoulos
openaire   +5 more sources

Dawes Review 4: Spiral Structures in Disc Galaxies [PDF]

open access: yesPublications Astronomical Society of Australia, 2014
The majority of astrophysics involves the study of spiral galaxies, and stars and planets within them, but how spiral arms in galaxies form and evolve is still a fundamental problem. Major progress in this field was made primarily in the 1960s, and early
C. Dobbs, J. Baba
semanticscholar   +4 more sources

Updating the (Supermassive Black Hole Mass) - (Spiral Arm Pitch Angle) Relation: A Strong Correlation for Galaxies with Pseudobulges [PDF]

open access: yes, 2017
We have conducted an image analysis of the (current) full sample of 44 spiral galaxies with directly measured supermassive black hole (SMBH) masses, $M_{\rm BH}$, to determine each galaxy's logarithmic spiral arm pitch angle, $\phi$. For predicting black
Benjamin Lee Davis, A. Graham, M. Seigar
semanticscholar   +3 more sources

Reanalysis of the Spin Direction Distribution of Galaxy Zoo SDSS Spiral Galaxies

open access: yesAdvances in Astronomy, 2023
The distribution of the spin directions of spiral galaxies in the Sloan Digital Sky Survey has been a topic of debate in the past two decades, with conflicting conclusions reported even in cases where the same data were used.
Darius Mcadam, Lior Shamir
doaj   +1 more source

Spirality: A Novel Way to Measure Spiral Arm Pitch Angle

open access: yesGalaxies, 2022
We present the MATLAB code Spirality, a novel method for measuring spiral arm pitch angles by fitting galaxy images to spiral templates of known pitch. Computation time is typically on the order of 2 min per galaxy, assuming 8 GB of working memory.
Deanna Shields   +9 more
doaj   +1 more source

Discovery of a Planar Black Hole Mass Scaling Relation for Spiral Galaxies

open access: yesThe Astrophysical Journal Letters, 2023
Supermassive black holes (SMBHs) are tiny in comparison to the galaxies they inhabit, yet they manage to influence and coevolve along with their hosts.
Benjamin L. Davis, Zehao Jin
doaj   +1 more source

SDSS-IV MaNGA: global stellar population and gradients for about 2000 early-type and spiral galaxies on the mass-size plane [PDF]

open access: yes, 2018
We perform full spectrum fitting stellar population analysis and Jeans Anisotropic modelling (JAM) of the stellar kinematics for about 2000 early-type galaxies (ETGs) and spiral galaxies from the MaNGA DR14 sample.
Hongyu Li   +14 more
semanticscholar   +1 more source

On the plausible origins of the spiral character of galaxies

open access: yesOpen Astronomy, 2021
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

Shape of the oxygen abundance profiles in CALIFA face-on spiral galaxies [PDF]

open access: yes, 2016
We measured the gas abundance profiles in a sample of 122 face-on spiral galaxies observed by the CALIFA survey and included all spaxels whose line emission was consistent with star formation.
L. Sánchez-Menguiano   +33 more
semanticscholar   +1 more source

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