Issue |
A&A
Volume 520, September-October 2010
|
|
---|---|---|
Article Number | A41 | |
Number of page(s) | 7 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201014329 | |
Published online | 28 September 2010 |
Implications of a new triple-α nuclear reaction rate
Consequences for Cepheids
1
Université de Nice-Sophia Antipolis, CNRS UMR 6202,
Observatoire de la Côte d'Azur, Laboratoire Cassiopée,
BP 4229, 06304 Nice Cedex 04, France e-mail: [Pierre.Morel;Janine.Provost;Bernard.Pichon;Frederic.Thevenin]@oca.eu
2
Observatoire de Paris, Laboratoire GEPI,
CNRS UMR 8111, 92195 Meudon, France e-mail: Yveline.Lebreton@obspm.fr
3
IPR, Université de Rennes 1, 35042 Rennes, France e-mail: Yveline.Lebreton@univ-rennes1.fr
Received:
26
February
2010
Accepted:
13
June
2010
Context. Recently the triple-α reaction rate has been re-evaluated. In the temperature range, 107–108 K, with respect to the NACRE rate, the new rate is enhanced by up to 20 orders-magnitude.
Aims. To validate this new rate, we investigate its consequences for the evolution of Cepheid models.
Methods. The stellar evolutionary tracks are calculated with the CESAM code
and displayed in the domain 4–10 .
Results. With the new rate, the first dredge-up does not occur.
For masses larger than 4.5
each evolutionary
track crosses the instability strip only once. The luminosities are higher
than with the previous rate, then leading to smaller theoretical masses that
better agree with the pulsational mass. Conversely, and inconsistently with one
century of observations of more than two hundred
Cepheids, the temporal derivative of the period keeps a positive sign.
Moreover the observed depletions of atmospheric lithium and C/N ratio do not
occur. A slight modification of only a few percents of the
new nuclear rate allows us however to restore the loops inside the instability
strip and the changes of sign of the temporal derivative of periods.
Conclusions. This preliminary work indicates that the new rate may solve some of the long-lasting unsolved theoretical problems of Cepheids. Yet indisputable observations argue against its pertinence. Nonetheless, with regard to its theoretical importance, the triple-α new reaction rate still needs to be confirmed or revisited.
Key words: nuclear reactions / nucleosynthesis / abundances / stars: evolution / stars: variables: Cepheids
© ESO, 2010
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