[PDF] from arxiv.org…, M Beck, N Mowlavi, P De Cat… - Monthly Notices of …, 2011 - Wiley Online Library P. Dubath,1,2⋆ L. Rimoldini,1,2 M. Süveges,1,2 J. Blomme,3 M. López,4 LM Sarro,5 J. De Ridder,3 J. Cuypers,6 L. Guy,1,2 I. Lecoeur,1,2 K. Nienartowicz,1,2 A. Jan,1,2 M. Beck,1,2 N. Mowlavi,1,2 P. De Cat,6 T. Lebzelter7 and L. Eyer1,2 1Observatoire astronomique de l' ... Cited by 3 - Related articles - All 5 versions
[PDF] from arxiv.org…, M Briquet, T Morel, P De Cat - The Astrophysical …, 2011 - iopscience.iop.org S. HUBRIG1, I. ILYIN1, M. SCHÖLLER2, M. BRIqUET3, T. MOREL4, AND P. DE CAT5 1 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany; shubrig@aip.de 2 European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, ... Cited by 6 - Related articles - All 11 versions
SCAT Davis, BE Westerhof… - Journal of …, 2011 - journals.lww.com Wolters Kluwer Health may email you for journal alerts and information, but is committed to maintaining your privacy and will not share your personal information without your express consent. For more information, please refer to our Privacy Policy. ... Skip Navigation Links Home > Current ... Cited by 2 - Related articles - All 4 versions
…, D Shulyak, V Tsymbal, P De Cat - Astronomy & …, 2011 - aanda.org Results. We determine T eff , log g, microturbulent velocity, vsini, metallicity, and elemental abundance for 14 of the 16 candidate stars. Two stars are spectroscopic binaries. No significant influence of NLTE effects on the results could be found. For hot stars, we find systematic deviations ... Cited by 2 - Related articles - All 6 versions
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