Results 131 to 140 of about 8,504 (230)

The TYPHOON Stellar Population Synthesis Survey. II. Pushing Full Spectral Fitting to the Limit in the Nearby Grand Design Barred Spiral M83

open access: yesThe Astrophysical Journal
We apply population synthesis techniques to analyze TYPHOON long slit spectra of the starburst barred spiral galaxy M83. The analysis covers a central square of 5′ side length.
Eva Sextl   +9 more
doaj   +1 more source

Stellar and gas dynamics of late-type barred-spiral galaxies: NGC 3359, a test case [PDF]

open access: bronze, 2009
P. A. Patsis   +3 more
openalex   +1 more source

Effects of Halo Spin on the Formation and Evolution of Bars in Disk Galaxies

open access: yesThe Astrophysical Journal
The spin of dark halos has been shown to significantly affect bar formation and evolution in disk galaxies. To understand the physical role of halo spin in bar formation, we run N -body simulations of isolated, Milky Way–sized galaxies by varying the ...
Dajeong Jang, Woong-Tae Kim
doaj   +1 more source

H [CSC]i[/CSC] Observations of the Spiral Arm Pattern Speed in the Late-Type Barred Galaxy NGC 925 [PDF]

open access: green, 1998
Bruce G. Elmegreen   +5 more
openalex   +1 more source

Automated Detection of Galactic Rings from Sloan Digital Sky Survey Images

open access: yesThe Astrophysical Journal
Morphological features in galaxies—like spiral arms, bars, rings, and tidal tails, etc.—carry information about their structure, origin, and evolution.
Linn Abraham   +6 more
doaj   +1 more source

Determination of the Pattern Speed of Barred Spiral Galaxies [PDF]

open access: bronze, 2009
Akihiko Hirota   +7 more
openalex   +1 more source

High-velocity Molecular Clouds in M83

open access: yesThe Astrophysical Journal
High-velocity clouds (HVCs), which are gas clouds moving at high velocity relative to the galactic disk, may play a critical role in galaxy evolution, potentially supplying gas to the disk and triggering star formation.
Maki Nagata   +6 more
doaj   +1 more source

Tracing Coherent Gas Structures in the Central Region of the Starburst Galaxy NGC 253. II. Gas Excitation and Star Formation

open access: yesThe Astrophysical Journal
Molecular gas in the central region of the starburst galaxy NGC 253 is complicated because of the combination of different gas kinematics, including stellar feedback, noncircular motions, and magnetic activity.
Ryotaro Konishi   +5 more
doaj   +1 more source

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