Die Autorin dieses Werkes

Maria Fernanda Nieva Bamberg, Germany

Biographie:

María Fernanda Nieva was born in 1974 in Tucumán, Argentina. The studies of physics at the Universidad Nacional de Tucumán were accomplished in 2002, with the diploma thesis: "Determinación de Temperatura Efectiva y Estado de Evolución de Estrellas tipo B, A y F". The Ph.D. study on quantitative spectroscopy of OB stars was made in a cotutelle programme between Observatório Nacional (Brazil) and the Friedrich-Alexander-Universität Erlangen-Nürnberg (Germany). To date she is (co-)author of 10 scientific papers in refereed journals and conference proceedings.

Publikationen im VerkanntenVerlag:

Quantitative Spectroscopy of OB Stars Hydrogen, Helium and Carbon
Dissertation [Wissenschaft] 23. 10. 2007  150 S.  Buch  ISBN: 978-3-00-023064-6   VVPN: 00001008

Weitere Veröffentlichungen:

Nieva, M.F. 2002, Determinacion de Temperatura Efectiva y Estado de Evolucion de Estrellas Tipo B, A y F", Diploma Thesis, Universidad Nacional de Tucuman, Argentina

Nieva, M.F. & Przybilla, N. 2006a, C II Abundances in Early-Type Stars: Solution to a Notorious Non-LTE Problem, ApJL, 639, L39

Nieva, M.F. & Przybilla, N. 2006b, Present-Day Carbon Abundances of Early-Type Stars, in: Nuclei in Cosmos IX, Proceedings of Science, PoS(NIC-IX)150 (astro-ph/060922)

Nieva, M.F. & Przybilla, N. 2007a, Hydrogen and helium line formation in OB dwarfs and giants. A hybrid non-LTE approach, A&A, 467, 295

Nieva, M.F. & Przybilla, N. 2007b, Accurate Quantitative Spectroscopy of OB Stars: the H, He and C Spectrum, in: Precision Spectroscopy in Astrophysics, Springer-Verlag, in press

Nieva, M.F. & Przybilla, N. 2007c, Accurate Quantitative Spectroscopy of OB Stars: C and N abundances near the Main Sequence, in: Massive Stars. Fundamental Parameters and Circumstellar Interactions, RMxAA Conf. Ser., in press

Nieva, M.F. & Przybilla, N. 2007d, Non-LTE line-formation for C II-IV in early B-type stars. Self-consistent stellar atmospheric parameters and a reevaluation of the present-day carbon abundance in the solar neighbourhood, submitted to A&A

Adelman, S.J., Pintado, O.I., Nieva, F., et al. 2002, On the effective temperatures and surface gravities of superficially normal main sequence B and A stars, A&A, 392, 1031


Korn, A.J., Nieva, M.F. Daflon, S., & Cunha, K. 2005, Pristine CNO Abundances from Magellanic Cloud B Stars. II. Fast Rotators in the Large Magellanic Cloud Cluster NGC 2004, ApJ, 633, 899

Przybilla, N., Nieva, M.F., & Edelmann, H. 2006, NLTE Analyses of SdB Stars: Progress and Prospects, Baltic Astronomy, 15, 107

Przybilla, N., Nieva, M.F., Heber, U., & Jeffery, C.S. 2006, Non-LTE Metal Abundances in V652 HER and HD 144941, Baltic Astronomy, 15, 163