Contact Binaries with Additional Components. I. The Extant Data

By T. Pribulla, S. Rucinski. 2006

231 citations recorded by the source corpus.

We have attempted to establish observational evidence for the presence of distant companions that may have acquired and/or absorbed angular momentum during the evolution of multiple systems, thus facilitating or enabling the formation of contact binaries. In this preliminary investigation we use several techniques (some of them distance-independent) and mostly disregard the detection biases of individual techniques in an attempt to establish a lower limit to the frequency of triple systems. While the whole sample of 151 contact binary stars brighter than Vmax = 10 mag gives a firm lower limit of 42% ± 5%, the corresponding number for the much better observed northern-sky subsample is 59% ± 8%. These estimates indicate that most contact binary stars exist in multiple systems.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/b43f2cdeaafd9435649938db51373c3a0fd65fe7

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In Astronomy and Astrophysics

  1. S. Naoz
  2. B. Kocsis
  3. T. Thompson
  4. Abraham Loeb
  5. H. Perets
  6. F. Antonini
  7. F. Rasio
  8. D. Fabrycky

In Instrumentation

  1. S. Naoz
  2. B. Kocsis
  3. T. Thompson
  4. Abraham Loeb
  5. H. Perets
  6. D. Fabrycky
  7. T. Mazeh
  8. N. Yunes

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