M 82 - NGC 3034

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Models, Galaxies, Filaments, Galactic Structure, Hydrogen, Radial Velocity

Scientific paper

The development of theories concerning the nature of the galaxy M 82 is reviewed. The significance of the system of filaments extending from the center of the galaxy and of the dust cloud surrounding the galaxy is addressed. A model that explains these phenomena as well as the broadband radiation in the galactic core and the velocity gradients observed along the galaxy's minor axis is summarized.

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