The first confirmed microlens in a globular cluster

P. Pietrukowicz, D. Minniti, Ph Jetzer, J. Alonso-García, A. Udalski

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

16 Citas (Scopus)

Resumen

In 2000July/August a microlensing event occurred at a distance of 233 from the center of the globular cluster M22 (NGC 6656), observed against the dense stellar field of the Milky Way bulge. We have used the adaptive optics system NACO at the ESO Very Large Telescope to resolve the two objects that participated in the event: the lens and the source. The position of the objects measured in 2011July is in agreement with the observed relative proper motion of M22 with respect to the background bulge stars. Based on the brightness of the microlens components we find that the source is a solar-type star located at a distance of 6.0 1.5 kpc in the bulge, while the lens is a 0.18 0.01 M dwarf member of the globular cluster located at the known distance of 3.2 0.2 kpc from the Sun.

Idioma originalInglés
Número de artículoL18
PublicaciónAstrophysical Journal Letters
Volumen744
N.º2
DOI
EstadoPublicada - 10 ene. 2012

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica
  • Ciencias planetarias y espacial

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