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Thermohaline Mixing And Its Role In The Evolution Of Carbon And Nitrogen Abundances In Globular Cluster Red Giants: The Test Case Of Messier 3

In English

Författare

  • George C. Angelou
  • Ross Church
  • Richard J. Stancliffe
  • John C. Lattanzio
  • Graeme H. Smith

Summary, in English

We review the observational evidence for extra mixing in stars on the red giant branch (RGB) and discuss why thermohaline mixing is a strong candidate mechanism. We recall the simple phenomenological description of thermohaline mixing and aspects of mixing in stars in general. We use observations of M3 to constrain the form of the thermohaline diffusion coefficient and any associated free parameters. This is done by matching [C/Fe] and [N/Fe] along the RGB of M3. After taking into account a presumed initial primordial bimodality of [C/Fe] in the CN-weak and CN-strong stars, our thermohaline mixing models can explain the full spread of [C/Fe]. Thermohaline mixing can produce a significant change in [N/Fe] as a function of absolute magnitude on the RGB for initially CN-weak stars, but not for initially CN-strong stars, which have so much nitrogen to begin with that any extra mixing does not significantly affect the surface nitrogen composition.

Publiceringsår

2011

Språk

Engelska

Publikation/Tidskrift/Serie

Astrophysical Journal

Volym

728

Issue

2

Dokumenttyp

Artikel i tidskrift

Förlag

American Astronomical Society

Ämne

  • Astronomy, Astrophysics and Cosmology

Nyckelord

  • globular clusters: individual (M3)
  • stars: abundances
  • stars:
  • evolution
  • stars: Population II

Status

Published

ISBN/ISSN/Övrigt

  • ISSN: 0004-637X