Microlensing by gas filaments
arXiv:astro-ph/0409720 · doi:10.1111/j.1365-2966.2004.08454.x
Abstract
Gas in the interstellar matter is generally organized in filamentary structures, which may be also relevant for a complementary explanation of the dark matter in the Galactic halo. We examine the possibility that such structures may act as gravitational microlenses on background sources. To this purpose, we derive the general properties of a cylindrical lens and compare the light curves produced by such microlensing events with those generated by spherically symmetric clouds. We find that the establishment of the symmetry of the lens through the sole analysis of the light curve may be problematic, while the analysis of the astrometric shift of the centroid of the image can discriminate between the two classes of clouds. On the basis of our analysis, we find that only gas filaments with a very high density could be detectable. Such clouds are unlikely to exist in a long-lived state. Therefore, microlensing cannot discriminate on the existence and the relevance of gas filaments in the Halo, which could well be present and escape detection by ordinary microlensing surveys.
11 pages, 6 figures, in press on MNRAS
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