Gravitational microlensing events due to stellar-mass black holes

D. P. Bennett, A. C. Becker, J. L. Quinn, A. B. Tomaney, C. Alcock, R. A. Allsman, D. R. Alves, T. S. Axelrod, J. J. Calitz, K. H. Cook, A. J. Drake, P. C. Fragile, K. C. Freeman, M. Geha, K. Griest, B. R. Johnson, S. C. Keller, C. Laws, M. J. Lehner, S. L. MarshallD. Minniti, C. A. Nelson, B. A. Peterson, P. Popowski, M. R. Pratt, P. J. Quinn, S. H. Rhie, C. W. Stubbs, W. Sutherland, T. Vandehei, D. Welch

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86 Citas (Scopus)

Resumen

We present an analysis of the longest timescale microlensing events discovered by the MACHO Collaboration during a 7 year survey of the Galactic bulge. We find six events that exhibit very strong microlensing parallax signals due, in part, to accurate photometric data from the GMAN and MPS collaborations. The microlensing parallax fit parameters are used in a likelihood analysis, which is able to estimate the distances and masses of the lens objects based on a standard model of the Galactic velocity distribution. This analysis indicates that the most likely masses of five of the six lenses are greater than 1 M, which suggests that a substantial fraction of the Galactic lenses may be massive stellar remnants. This could explain the observed excess of long-timescale microlensing events. The lenses for events MACHO-96-BLG-5 and MACHO-98-BLG-6 are the most massive, with mass estimates of M / M = 6-3+10 and M / M = 6-3+7, respectively. The observed upper limits on the absolute brightness of main-sequence stars for these lenses are less than 1 L, so both lenses are black hole candidates. The black hole interpretation is also favored by a likelihood analysis with a Bayesian prior using a conventional model for the lens mass function. We consider the possibility that the source stars for some of these six events may lie in the foreground Galactic disk or in the Sagittarius (Sgr) dwarf galaxy behind the bulge, but we find that bulge sources are likely to dominate our microlensing parallax event sample. Future Hubble Space Telescope observations of these events can either confirm the black hole lens hypothesis or detect the lens stars and provide a direct measurement of their masses. Future observations of similar events by the Space Interferometry Mission or the Keck or VLT interferometers, as explained by Delplancke, Górski, & Richichi, will allow direct measurements of the lens masses for stellar remnant lenses as well.

Idioma originalInglés
Páginas (desde-hasta)639-659
Número de páginas21
PublicaciónAstrophysical Journal
Volumen579
N.º2 I
DOI
EstadoPublicada - 10 nov 2002

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica
  • Ciencias planetarias y espacial

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