Variability of the EROS no. 2 microlensing candidate.

Details Variability of the EROS no. 2 microlensing candidate. Variability of the EROS no. 2 microlensing candidate.

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...299l..21a&link_type=abstract

Astronomy and Astrophysics, v.299, p.L21

Astronomy and Astrophysics

Astrophysics

33

Accretion, Dark Matter, Microlensing, Variable Stars: Cataclysmic, Binaries: Eclipsing

Scientific paper

In this letter we report the analysis of data concerning the EROS no. 2
microlensing candidate. We have performed photometric measurements on
this star using three different telescopes. It was found to exhibit a
periodic variability. This source could be an eclipsing binary system,
of period 2.8 days.

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