Intergalactic dust near NGC 300

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Cosmic Dust, Galaxies, Hydrogen Clouds, Intergalactic Media, Optical Thickness, Astronomical Models, Radial Velocity, Stellar Evolution

Scientific paper

A search by means of galaxy counts for obscuring dust in an intergalactic hydrogen cloud near NGC 300 has resulted in the detection of a significant optical depth equal to 0.09 plus or minus 0.01. If the size and composition of the dust is similar to Galactic material, the implied dust to gas ratio is only about a factor of three smaller than the Galactic value.

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