The binary fraction of the young cluster NGC 1818 in the Large Magellanic Cloud

Y. Hu*, L. Deng, Richard de Grijs, Q. Liu, Simon P. Goodwin

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

18 Citations (Scopus)

Abstract

We use high-resolution Hubble Space Telescope imaging observations of the young (∼ 15-25 Myr old) star cluster NGC 1818 in the Large Magellanic Cloud to derive an estimate for the binary fraction of F stars (1.3 < M */M < 1.6). This study provides the strongest constraints yet on the binary fraction in a young star cluster in a low-metallicity environment ([Fe/H] ∼ -0.4 dex). Employing artificial-star tests, we develop a simple method that can efficiently measure the probabilities of stellar blends and superpositions from the observed stellar catalog. We create synthetic color-magnitude diagrams matching the fundamental parameters of NGC 1818, with different binary fractions and mass-ratio distributions. We find that this method is sensitive to binaries with mass ratios q ≳ 0.4. For binaries with F-star primaries and mass ratios q > 0.4, the binary fraction is ∼0.35. This suggests a total binary fraction for F stars of 0.55 to unity, depending on assumptions about the form of the mass-ratio distribution at low q.

Original languageEnglish
Pages (from-to)649-656
Number of pages8
JournalAstrophysical Journal
Volume724
Issue number1
DOIs
Publication statusPublished - 20 Nov 2010
Externally publishedYes

Keywords

  • binaries: general
  • galaxies: star clusters: general
  • Magellanic Clouds
  • methods: statistical

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