Results 211 to 220 of about 184,560 (234)
Virgo High-Resolution CO Survey: IV. Spiral-Driven Gas Dynamics in the Non-Barred Seyfert Galaxy NGC 4501 [PDF]
Sachiko Onodera+3 more
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The Dark Matter Content of Barred Spiral Galaxies [PDF]
G. Petitpas+3 more
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ASTE CO(3-2) Observations of the Southern Barred Spiral Galaxy NGC 986: a Large Gaseous Bar Filled with a Dense Molecular Medium [PDF]
Kotaro Kohno+23 more
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MeerKAT discovery of an infalling cold gas tail onto the nearby barred spiral galaxy, NGC 5643
Karina C Santana+3 more
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Starbursts in barred spiral galaxies IV: On young bars and the formation of abundance gradients
S. Considère+3 more
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High Resolution Neutral Hydrogen Observations of the Barred Spiral Galaxy NGC 1365
S. Jorsater, G. V. Moorsel
semanticscholar +1 more source
Dynamical Models of the Barred Spiral Galaxy NGC 3992
J. Hunter+4 more
semanticscholar +1 more source
Quantitative Morphology of Bars in Spiral Galaxies
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Physics Letters A, 2000
Abstract Here we put forward some arguments in favour of the existence of slow bars. More then a half of spiral galaxies have in their central regions a bar — a structure in the form of triaxial ellipsoid. Historically two models of the bar were developed — those of the so called “slow” and “fast” bars. In both cases the bar is in some resonance with
A.M. Fridman, O.V. Khoruzhii
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Abstract Here we put forward some arguments in favour of the existence of slow bars. More then a half of spiral galaxies have in their central regions a bar — a structure in the form of triaxial ellipsoid. Historically two models of the bar were developed — those of the so called “slow” and “fast” bars. In both cases the bar is in some resonance with
A.M. Fridman, O.V. Khoruzhii
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The barred spiral structure of galaxies
Chinese Astronomy and Astrophysics, 1984Abstract We have carried out a preliminary analysis of barred spirals using a gas-dynamical model. By means of the method of integral transform given in a previous paper [1], an analytical solution has been obtained which is in fair agreement with observations.
Xu Mei, Chen Zhen-cheng, Weng Shi-da
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