Results 141 to 150 of about 184,560 (234)
A catalogue of the morphological features for the complete Spitzer Survey of Stellar Structure in Galaxies (S$^4$G), including 2352 nearby galaxies, is presented.
Díaz-García, S.+3 more
core +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
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
doaj +1 more source
Ring Star Formation Rates in Barred and Nonbarred Galaxies
Nonbarred ringed galaxies are relatively normal galaxies showing bright rings of star formation in spite of lacking a strong bar. This morphology is interesting because it is generally accepted that a typical ring forms when material collects near a ...
Athanassoula+54 more
core +1 more source
Effects of Halo Spin on the Formation and Evolution of Bars in Disk Galaxies
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
Double-Barred Galaxies: I. A Catalog of Barred Galaxies with Stellar Secondary Bars and Inner Disks
I present a catalog of 67 barred galaxies which contain distinct, elliptical stellar structures inside their bars. Fifty of these are double-barred galaxies: a small-scale, "inner" or "secondary" bar is embedded within a large-scale, "outer" or "primary"
Afanasiev+128 more
core +1 more source
The Milky Way (MW) is a barred spiral galaxy shaped by tidal interactions with its satellites. The Large Magellanic Cloud (LMC) and the Sagittarius dwarf galaxy (Sgr) are the dominant influences at the present day. This paper presents a suite of four 10 ^
Ioana A. Stelea+2 more
doaj +1 more source
Inner Workings: Astronomers are redrawing our corner of the Milky Way. [PDF]
Croswell K.
europepmc +1 more source
The kinematics and structure of the neutral hydrogen in the barred spiral galaxy NGC 3359.
The barred spiral galaxy NGC 3359 has been observed with the three-element line interferometer of the National Radio Astronomy Observatory. An angular resolution of 42'' x 31'' was achieved with a velocity resolution of 24.5 km/s.
S. Gottesman
semanticscholar +1 more source
Astronomia ex machina: a history, primer and outlook on neural networks in astronomy. [PDF]
Smith MJ, Geach JE.
europepmc +1 more source