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Toward Understanding the B[e] Phenomenon. VII. AS 386, a Single-lined Binary with a Candidate Black Hole Component

  • S. A. Khokhlov
  • , A. S. Miroshnichenko
  • , S. V. Zharikov
  • , N. Manset
  • , A. A. Arkharov
  • , N. Efimova
  • , S. Klimanov
  • , V. M. Larionov
  • , A. V. Kusakin
  • , R. I. Kokumbaeva
  • , Ch T. Omarov
  • , K. S. Kuratov
  • , A. K. Kuratova
  • , R. J. Rudy
  • , E. A. Laag
  • , K. B. Crawford
  • , T. K. Swift
  • , R. C. Puetter
  • , R. B. Perry
  • , S. D. Chojnowski
  • A. Agishev, D. B. Caton, R. L. Hawkins, A. B. Smith, D. E. Reichart, V. V. Kouprianov, J. B. Haislip
  • Al-Farabi Kazakh National University
  • Fesenkov Astrophysical Institute
  • University of North Carolina at Greensboro
  • Universidad Nacional Autónoma de México
  • CFHT Corporation
  • Russian Academy of Sciences
  • VNIIOkeangeologia and St. Petersburg State University
  • Aerospace Corporation, USA
  • Massachusetts Institute of Technology
  • University of California San Diego
  • NASA Langley Research Center
  • Apache Point Observatory
  • Department of Physics and Astronomy
  • Appalachian State University
  • Gemini Observatory
  • University of North Carolina at Chapel Hill

Research output: Contribution to journalArticlepeer-review

Original languageEnglish
Article number158
JournalAstrophysical Journal
Volume856
Issue number2
DOIs
StatePublished - Apr 1 2018

ASJC Scopus Subject Areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • binaries: spectroscopic
  • stars: emission-line, Be
  • stars: individual (AS 386)

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