Die Autorin dieses Werkes

Maria Fernanda Nieva
Bamberg, Germany


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