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  • Brogaard, K.Aarhus University,University of Birmingham (author)

The blue straggler V106 in NGC6791 : A prototype progenitor of old single giants masquerading as young

  • Article/chapterEnglish2018

Publisher, publication year, extent ...

  • 2018
  • 11 s.

Numbers

  • LIBRIS-ID:oai:lup.lub.lu.se:aa197dba-0e92-493f-a464-8faada673cbb
  • https://lup.lub.lu.se/record/aa197dba-0e92-493f-a464-8faada673cbbURI
  • https://doi.org/10.1093/MNRAS/STY2504DOI

Supplementary language notes

  • Language:English
  • Summary in:English

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  • Subject category:art swepub-publicationtype
  • Subject category:ref swepub-contenttype

Notes

  • We determine the properties of the binary star V106 in the old open cluster NGC6791. We identify the system to be a blue straggler cluster member by using a combination of groundbased and Kepler photometry and multi-epoch spectroscopy. The properties of the primary component are found to be Mp ~ 1.67M⊙, more massive than the cluster turn-off, with Rp ~ 1.91R⊙ and Teff = 7110 ± 100 K. The secondary component is highly oversized and overluminous for its low mass with Ms ~ 0.182M⊙, R⊙ ~ 0.864R⊙, and T⊙ =6875±200 K. We identify this secondary star as a bloated (proto) extremely low-mass helium white dwarf. These properties of V106 suggest that it represents a typical Algol-paradox system and that it evolved through a mass-transfer phase, which provides insight into its past evolution. We present a detailed binary stellar evolution model for the formation of V106 using the MESA code and find that the mass-transfer phase only ceased about 40 Myr ago. Due to the short orbital period (P = 1.4463 d), another mass-transfer phase is unavoidable once the current primary star evolves towards the red giant phase. We argue that V106 will evolve through a common-envelope phase within the next 100 Myr and merge to become a single overmassive giant. The high mass will make it appear young for its true age, which is revealed by the cluster properties. Therefore, V106 is potentially a prototype progenitor of old field giants masquerading as young.

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Added entries (persons, corporate bodies, meetings, titles ...)

  • Christiansen, S. M.Aarhus University (author)
  • Grundahl, F.Aarhus University (author)
  • Miglio, A.University of Birmingham,Aarhus University (author)
  • Izzard, R. G.University of Surrey (author)
  • Tauris, T. M.University of Bonn,Max Planck Institute for Radio Astronomy,Aarhus University (author)
  • Sandquist, E. L.San Diego State University (author)
  • Vanden Berg, D. A.University of Victoria (author)
  • Jessen-Hansen, J.Aarhus University (author)
  • Arentoft, T.Aarhus University (author)
  • Bruntt, H.Aarhus University (author)
  • Frandsen, S.Aarhus University (author)
  • Orosz, J. A.San Diego State University (author)
  • Feiden, G. A.Uppsala University (author)
  • Mathieu, R.University of Wisconsin-Madison (author)
  • Geller, A.University of Wisconsin-Madison (author)
  • Shetrone, M.University of Texas System (author)
  • Ryde, N.Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science(Swepub:lu)astr-nlr (author)
  • Stello, D.University of New South Wales,University of Sydney,Aarhus University (author)
  • Platais, I.Johns Hopkins University (author)
  • Meibom, S.Harvard–Smithsonian Center for Astrophysics (author)
  • Aarhus UniversityUniversity of Birmingham (creator_code:org_t)

Related titles

  • In:Monthly Notices of the Royal Astronomical Society481:4, s. 5062-50720035-8711

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