Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...185.1704c&link_type=abstract
American Astronomical Society, 185th AAS Meeting, #17.04; Bulletin of the American Astronomical Society, Vol. 26, p.1336
Astronomy and Astrophysics
Astronomy
Scientific paper
The MACHO project has recently completed the analysis of 24 Galactic bulge fields containing 1.3times 10(7) stars observed for 190 days. Approximately 45 microlensing events have been detected in this data set, and one of these events shows clear evidence of a "parallax" effect. That is, the effect of the earth's motion around the Sun can clearly be seen in the light curve. The event displayed an Einstein ring crossing time of ~ 108 days and a peak amplification of ~ 10x. The "parallax" induced asymmetry in the light curve enables us to determine a component of the velocity of the microlensing object with respect to the line connecting the Sun with the source star. The transverse component of this velocity projected to the position of the Sun is determined to be v_t ~ 54+/- 5 km/sec. This value and the timescale of the event can be used to show that the lensing event is probably due to lensing by a low mass star in the galactic disk or a brown dwarf in the galactic bulge. High resolution spectroscopy and multi-color photometry have been obtained and will provide constraints on the lens's distance and kinematic population.
Alcock Charles
Allsman Robyn
Axelrod Tim
Bennett Dave
Cook Kelly
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