ar X iv : a st ro - p h / 04 01 25 0 v 1 1 3 Ja n 20 04 MOA 2003 - BLG - 37 : A Bulge Jerk - Parallax Microlens Degeneracy

نویسندگان

  • D. L. DePoy
  • B. S. Gaudi
  • A. Gould
  • C. Han
  • B. - G. Park
  • R. W. Pogge
  • F. Abe
  • D. P. Bennett
  • I. A. Bond
  • S. Eguchi
  • Y. Furuta
  • J. B. Hearnshaw
  • K. Kamiya
  • P. M. Kilmartin
  • Y. Kurata
  • K. Masuda
  • Y. Matsubara
  • Y. Muraki
  • S. Noda
  • K. Okajima
  • N. J. Rattenbury
  • T. Sako
  • T. Sekiguchi
  • D. J. Sullivan
  • T. Sumi
  • P. J. Tristram
  • T. Yanagisawa
  • P. C. M. Yock
چکیده

– 2 – We analyze the Galactic bulge microlensing event MOA 2003-BLG-37. Although the Einstein timescale is relatively short, t E = 43 days, the lightcurve displays deviations consistent with parallax effects due to the Earth's accelerated motion. We show that the χ 2 surface has four distinct local minima that are induced by the " jerk-parallax " degeneracy, with pairs of solutions having projected Einstein radii, ˜ r E = 1.28 AU and 1.70 AU, respectively. This is the second event displaying such a degeneracy and the first toward the Galactic bulge. For both events, the jerk-parallax formalism accurately describes the offsets between the different solutions, giving hope that when extra solutions exist in future events, they can easily be found. However, the morphologies of the χ 2 surfaces for the two events are quite different, implying that much remains to be understood about this degeneracy.

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ar X iv : a st ro - p h / 04 01 25 0 v 2 14 M ar 2 00 4 MOA 2003 - BLG - 37 : A Bulge Jerk - Parallax Microlens Degeneracy

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تاریخ انتشار 2004