New:
I recently wrote a 9 page popular science article about the oldest stars (in German,
sorry) that will appear in the September 2008 issue of Spektrum der Wissenschaft. Check it out!
My primary research area is Galactic stellar astronomy:
I am interested in searching for the oldest stars in our Milky
Way Galaxy. By studying these stars, we can learn details about the nature
of the early Universe shortly after the Big Bang when the first
stars and galaxies began to form. Employing the the worlds largest optical
telescopes we identify old stars by means of their chemically primitive
nature. These so-called "metal-poor" stars contain only tiny amounts of
heavy elements ("metals") that are heavier than hydrogen and helium. They
formed before the Universe was significantly enriched in chemical elements,
as we know it today. Hence, the oldest stars in the Milky Way are stellar
fossils and make possible to reconstruct the chemical evolution of the
Galaxy from the earliest times until today.
A recent review on the metal-poor stars can be found here. It describes the role of metal-poor star
with regard to the early universe, the most recent discoveries, and how
these old objects help us to understand various nucleosynthesis processes
in stars, the origin of the elements and the chemical evolution of the
Galaxy.
This review is published in New Horizons in Astronomy: Frank N. Bash
Symposium 2007 ASP Conf. Ser., Vol. 393, eds. A. Frebel,
J. R. Maund, J. Shen, and M. H. Siegel. San Francisco: ASP, 2008, 63
Another review on r-process enhanced stars such as HE
1523-0901 which allow the detailed study of neutron-capture processes in
the cosmos can be found here. It will be
published in the proceedings of the "Nuclei in the Cosmos X" symposium, 2008.
I completed my PhD thesis "Abundance Analysis of Bright Metal-Poor
Stars from the Hamburg/ESO Survey" at the Research School of Astronomy &
Astrophysics of the Australian National
University located at Mt. Stromlo Observatory in Canberra, Australia. I
was supervised by John E. Norris (Australian Natl. Univ.), Mike S. Bessell
(Australian Natl. Univ.), Martin Asplund (Max-Planck Institute for
Astrophysics) and Norbert Christlieb (Landessternwarte Heidelberg).
If you would like to have a copy of my thesis, please send me an email
(address is given below).
I received the 2007 Charlene
Heisler Prize for the best PhD thesis in Astronomy, or a closely related field, accepted by an
Australian university in 2006.
Projects I'm currently leading:
Texas Stellar Archaeology Project: We use
metal-poor stars to learn about the first chemical enrichments, the initial
mass function, and the formation of the first low-mass objects in the
Universe
Previous projects (among others):
In 2004, one of my stars turned out to be the most iron-poor star known to date!
The hunt for the most metal-poor star: A quick history
Collaborators:
N. Christlieb (Sweden),
T.C. Beers (USA),
W. Aoki (Japan),
A. Korn (Sweden), and many others...
Our world leading team that finds the most metal-poor stars, at a scientific meeting in Paris, May 2005
left to right: W. Aoki (NAOJ), S. Ryan (Hertfordshire), M. Bessell (ANU), J. E. Norris (ANU),
M. Asplund (ANU), N. Christlieb (Heidelberg), T. Beers (MSU), A. Frebel (UT Austin)
Research Interest
Metal-poor stars, chemical abundances, abundance trends at the lowest metallicities, the r-process,
chemical evolution of the Galaxy, formation of the halo, high-resolution spectroscopy, ... and much more
Postal address:
Anna Frebel
The University of Texas
McDonald Observatory
1 University Station, C1402
Austin, Texas 78712-0259
USA
ph: +1 512 471 9985
fax: +1 512 471 6016
email: anna& at& astro. as. utexas. edu
last updated: August 2008
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