The Astrophysical Journal (Jan 2024)

First Resolution of Microlensed Images of a Binary-lens Event

  • Zexuan Wu,
  • Subo Dong,
  • A. Mérand,
  • Christopher S. Kochanek,
  • Przemek Mróz,
  • Jinyi Shangguan,
  • Grant Christie,
  • Thiam-Guan Tan,
  • Thomas Bensby,
  • Joss Bland-Hawthorn,
  • Sven Buder,
  • Frank Eisenhauer,
  • Andrew P. Gould,
  • Janez Kos,
  • Tim Natusch,
  • Sanjib Sharma,
  • Andrzej Udalski,
  • J. Woillez,
  • David A. H. Buckley,
  • I. B. Thompson,
  • Karim Abd El Dayem,
  • Anthony Berdeu,
  • Jean-Philippe Berger,
  • Guillaume Bourdarot,
  • Wolfgang Brandner,
  • Richard I. Davies,
  • Denis Defrère,
  • Catherine Dougados,
  • Antonia Drescher,
  • Andreas Eckart,
  • Maximilian Fabricius,
  • Helmut Feuchtgruber,
  • Natascha M. Förster Schreiber,
  • Paulo Garcia,
  • Reinhard Genzel,
  • Stefan Gillessen,
  • Gernot Heißel,
  • Sebastian Hönig,
  • Mathis Houlle,
  • Pierre Kervella,
  • Laura Kreidberg,
  • Sylvestre Lacour,
  • Olivier Lai,
  • Romain Laugier,
  • Jean-Baptiste Le Bouquin,
  • James Leftley,
  • Bruno Lopez,
  • Dieter Lutz,
  • Felix Mang,
  • Florentin Millour,
  • Miguel Montargès,
  • Hugo Nowacki,
  • Mathias Nowak,
  • Thomas Ott,
  • Thibaut Paumard,
  • Karine Perraut,
  • Guy Perrin,
  • Romain Petrov,
  • Pierre-Olivier Petrucci,
  • Nicolas Pourre,
  • Sebastian Rabien,
  • Diogo C. Ribeiro,
  • Sylvie Robbe-Dubois,
  • Matteo Sadun Bordoni,
  • Daryl Santos,
  • Jonas Sauter,
  • Jules Scigliuto,
  • Taro T. Shimizu,
  • Christian Straubmeier,
  • Eckhard Sturm,
  • Matthias Subroweit,
  • Calvin Sykes,
  • Linda Tacconi,
  • Frédéric Vincent,
  • Felix Widmann,
  • the GRAVITY+ collaboration

DOI
https://doi.org/10.3847/1538-4357/ad90b9
Journal volume & issue
Vol. 977, no. 2
p. 229

Abstract

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We resolve the multiple images of the binary-lens microlensing event ASASSN-22av using the GRAVITY instrument of the Very Large Telescope Interferometer (VLTI). The light curves show weak binary-lens perturbations, complicating the analysis, but the joint modeling with the VLTI data breaks several degeneracies, arriving at a strongly favored solution. Thanks to precise measurements of the angular Einstein radius θ _E = 0.724 ± 0.002 mas and microlens parallax, we determine that the lens system consists of two M dwarfs with masses of M _1 = 0.258 ± 0.008 M _⊙ and M _2 = 0.130 ± 0.007 M _⊙ , a projected separation of r _⊥ = 6.83 ± 0.31 au, and a distance of D _L = 2.29 ± 0.08 kpc. The successful VLTI observations of ASASSN-22av open up a new path for studying intermediate-separation (i.e., a few astronomical units) stellar-mass binaries, including those containing dark compact objects such as neutron stars and stellar-mass black holes.

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