1996International Astronomical Union ColloquiumOpen access

Inner Spiral Arms of the Barred Galaxy NGC 4314

Hong Bae Ann, Kideok Kwon

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Abstract

Abstract 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.

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Abstract 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.

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Available abstract

Abstract 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.

Key concepts: Barred spiral galaxy, Physics, Interacting galaxy, Unbarred spiral galaxy, Spiral galaxy, Grand design spiral galaxy, Astrophysics, Astronomy

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