A Search for a Near-Infrared Halo around NGC 4565

Astronomy and Astrophysics – Astronomy

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Cosmology: Dark Matter, Galaxies: Halos, Galaxies: Individual: Ngc Number: Ngc 4565, Stars: Low-Mass, Brown Dwarfs

Scientific paper

We present a near-infrared (3.5-5 μm) search for the integrated emission from low-mass stars and/or brown dwarfs in the halo of the nearby edge-on spiral galaxy NGC 4565. The observation was made with a liquid-helium-cooled rocket-borne telescope using a 256x256 InSb array with a pixel scale of 17". Images of NGC 4565 were successfully obtained with sensitivity near the natural background limit. Our search reveals no evidence of a faint halo around the galaxy, in contrast with the previous reports of a halo around NGC 5907. The lower limit of the mass-to-light ratio for the halo of NGC 4565 is 260 (2 sigma) in solar units at 3.5-5 mum. This implies that hydrogen-burning stars do not contribute significantly to the mass of the dark halo in NGC 4565.

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