Observation of Microlensing towards the Galactic Spiral Arms. EROS II 3 year survey

Abstract

We present an analysis of the light curves of 9.1 million stars observed during three seasons by EROS (Experience de Recherche d'Objets Sombres), in the Galactic plane away from the bulge. Seven stars exhibit luminosity variations compatible with gravitational microlensing effects due to unseen objects. The corresponding optical depth, averaged over four directions, is tau = 0.45 +0.24 -0.11 x 10^-6. While this value is compatible with expectations from simple galactic models under reasonable assumptions on the target distances, we find an excess of events with short timescale towards the direction closest to the Galactic Centre.

4 pages, 3 figures, submitted for publication in A&A Letters

References in corpus (4)

• The MACHO project: Microlensing Optical Depth towards the Galactic Bulge from Difference Image Analysis
• The Initial Mass Function of the Galactic Bulge Down to ~0.15 Msun
• Detection of the old stellar component of the major Galactic bar
• The properties of the Galactic bar implied by gas kinematics in the inner Milky Way

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