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Inner Spiral Arms of the Barred Galaxy NGC 4314

Published online by Cambridge University Press:  12 April 2016

H. B. Ann  and
K. H. Kwon
H. B. Ann*
Affiliation:
Department of Earth Sciences, Pusan National University, Pusan, 609-735, Korea
K. H. Kwon
Affiliation:
Department of Earth Sciences, Pusan National University, Pusan, 609-735, Korea
*
1Visiting Astronomer, Dominion Astrophysical Observatory.

Abstract

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The nuclear region of the barred galaxy NGC 4314 was observed and modeled by VIJHK photometry, long-slit spectroscopy, and SPH simulations. Young stellar populations is supposed to be made from the gas which are accumulated in the nuclear ring and/or inner spiral arms by the strong bar potential.

Type
Posters for Part I and Part II
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 88 - 90
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

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