Results 121 to 130 of about 7,946 (225)
Near-infrared surface photometry of barred spiral galaxies [PDF]
Claudia Baumgart, C. J. Peterson
openalex +1 more source
The Clearing Timescale for Infrared-selected Star Clusters in M83 with HST
We present an analysis of Hubble Space Telescope data from Wide Field Camera 3 (WFC3)/Ultraviolet Imaging Spectrometer, WFC3/IR, and the Advanced Camera for Surveys, investigating the young stellar cluster (YSC) population in the face-on spiral galaxy ...
Suyash Deshmukh +8 more
doaj +1 more source
The Formation of Nuclear Rings in Barred Spiral Galaxies [PDF]
Michael W. Regan +3 more
openalex +1 more source
Formation Mechanisms for Spirals in Barred Galaxies
We consider a scenario of formation of the spiral structure in barred galaxies. This scenario includes the new non-resonant mechanism of elongation of spirals, due to the characteristic behaviour of the gravitational potential beyond the principal spiral arms.
Polyachenko, Evgenii V. +1 more
openaire +2 more sources
Ring or No Ring—Revisiting the Multiphase Nuclear Environment in M31
Nuclear rings, prevalent in barred galaxies, are essential to understanding gas transport toward galactic nuclei. However, the peculiar nuclear ring in our neighboring galaxy M31 remains poorly understood.
Zongnan Li +11 more
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Enhanced star formation: The importance of bars in spiral galaxies [PDF]
It was found that among an IR luminous subset of nearby spiral galaxies, nearly all of the systems with IRAS colors and luminosities indicative of enhanced star formation are barred.
Hawarden, T. G. +3 more
core +1 more source
Radio Continuum Maps of Southern Barred Spiral Galaxies [PDF]
Margaret Mazzolini +2 more
openalex +1 more source
Orbital Support and Evolution of CX/OX Structures in Boxy/Peanut Bars
Barred galaxies exhibit boxy/peanut or X-shapes (BP/X) protruding from their disks in edge-on views. Two types of BP/X morphologies exist depending on whether the X-wings meet at the center (CX) or are off-centered (OX).
Behzad Tahmasebzadeh +9 more
doaj +1 more source
Stellar and gas dynamics of late-type barred-spiral galaxies: NGC 3359, a test case [PDF]
P. A. Patsis +3 more
openalex +1 more source
Bar structures can form internally due to the instability of their host galaxies or externally due to perturbations from other galaxies. We systematically quantify the growth timescales ( Ď„ _bar ) of bars formed through these two mechanisms with a series
Yirui Zheng +3 more
doaj +1 more source

