The binary nature of an observed dark galactic object

Details The binary nature of an observed dark galactic object The binary nature of an observed dark galactic object

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...289l..31d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 289, no. 1, p. L31-L33

Astronomy and Astrophysics

Astrophysics

29

Asymmetry, Binary Stars, Brown Dwarf Stars, Dark Matter, Gravitational Lenses, Light Curve, Magellanic Clouds, Data Correlation, Halos, Stellar Models, Stellar Spectrophotometry, Velocity

Scientific paper

The observed light curve of a star in the Large Magellanic Cloud (LMC)
published in Alcock et al. 1993 cannot be fitted to a symmetric light
curve due to gravitational microlensing by a single dark object in the
Galactic halo. We show that a binary lens producing an asymmetric light
curve can overcome the discepancy.

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