ISOCAM Observations of M31

Computer Science

Scientific paper

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Galaxies: Individual: M31, Galaxies: Ism

Scientific paper

We present ISOCAM images of the Andromeda galaxy center. They display an elliptical stellar bulge and a more complexe dust distribution. The spatial dust distribution follows a mini-spiral structure identical to the distribution of absorption in optical wavelengths. A discussion on the nature of the dust from CVF observations is also presented. The central part and the molecular ring of M31 are excellent targets for FIRST.

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