Observing molecular hydrogen clouds and dark massive objects in galactic halos

Details Observing molecular hydrogen clouds and dark massive objects in galactic halos Observing molecular hydrogen clouds and dark massive objects in galactic halos

1995-01-20

arxiv.org/abs/astro-ph/9501077v1

Astron.Astrophys.299:647,1995

Astronomy and Astrophysics

Astrophysics

7 pages, postscript file, to appear in Astron. & Astrophys

Scientific paper

Molecular hydrogen clouds can contribute substantially to the galactic halo< dark matter and may lead to the birth of massive halo objects (MHOs) observed indirectly by microlensing. We present a method to detect these molecular clouds in the halo of M31 using the Doppler shift effect. We also consider the possibility to directly observe MHOs in the halo of M31 via their infrared emission.

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