Volume 544, August 2012
|Number of page(s)||15|
|Section||Stellar structure and evolution|
|Published online||31 July 2012|
Nitrogen chronology of massive main sequence stars⋆
Argelander-Institut für Astronomie der Universität Bonn,
Auf dem Hügel 71,
2 University of Vienna, Department of Astronomy, Türkenschanzstr.17, 1180 Vienna, Austria
3 Astronomical Institute, Utrecht University, Princetonplein 5, 3584CC Utrecht, The Netherlands
4 Astronomical Institute Anton Pannekoek, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
Accepted: 12 June 2012
Context. Rotational mixing in massive main sequence stars is predicted to monotonically increase their surface nitrogen abundance with time.
Aims. We use this effect to design a method for constraining the age and the inclination angle of massive main sequence stars, given their observed luminosity, effective temperature, projected rotational velocity and surface nitrogen abundance.
Methods. This method relies on stellar evolution models for different metallicities, masses and rotation rates. We use the population synthesis code STARMAKER to show the range of applicability of our method.
Results. We apply this method to 79 early B-type main sequence stars near the LMC clusters NGC 2004 and N 11 and the SMC clusters NGC 330 and NGC 346. From all stars within the sample, 17 were found to be suitable for an age analysis. For ten of them, which are rapidly rotating stars without a strong nitrogen enhancement, it has been previously concluded that they did not evolve as rotationally mixed single stars. This is confirmed by our analysis, which flags the age of these objects as highly discrepant with their isochrone ages. For the other seven stars, their nitrogen and isochrone ages are found to agree within error bars, what validates our method. Constraints on the inclination angle have been derived for the other 62 stars,with the implication that the nitrogen abundances of the SMC stars, for which mostly only upper limits are known, fall on average significantly below those limits.
Conclusions. Nitrogen chronology is found to be a new useful tool for testing stellar evolution and to constrain fundamental properties of massive main sequence stars. A web version of this tool is provided.
Key words: stars: massive / stars: evolution / stars: rotation / stars: abundances / stars: early-type
Appendices are available in electronic form at http://www.aanda.org
© ESO, 2012
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