John
Cowan - cowan@mail.nhn.ou.edu
Poster and Press Release from Washington AAS Meeting.
Pdf version with color figures: The Extremely Metal-Poor, Neutron-Capture Rich Star CS 22892--052: A Comprehensive Abundance Analysis, astro-ph/0303542, Astrophys. J., 591, 936 (2003).
Pdf version with color figures: Binary Blue Metal-Poor Stars: Evidence for AGB Mass Transfer, astro-ph/0304064, Astrophys. J., 592, 504 (2003).
Pdf version : Elements of Surprise , Nature: News and Views, 423, 29 (May 4, 2003).
Pdf version : Galactic Evolution of Sr, Y and Zr: A Multiplicty of Nucleosynthetic Processes, Astrophys. J., 601, 864, (2004).
Pdf version : Improved Atomic Data for Ho II and New Holmium Abundances for the Sun and Three Metal-Poor Stars, Astrophys. J., 604, 850 (2004).
Pdf version : A Sprinkling of Stardust, Nature, 428, 369 (2004).
Pdf version : Stellar Abundances: The r-Process and Supernovae, in 3-D Signatures in Stellar Explosions, ed. P. Kumar, C. Wheeler & P. Hoeflich (Cambridge: Cambridge Univ. Press), 255 (2004).
Pdf version : Halo Star Abundances and Heavy Element Nucleosynthesis, astro-ph/0405423, in the Proceedings of the 12th Workshop on Nuclear Astrophysics, eds. E. Muller and H. Thomas Janka (Munich: MPI ), 41 (2004).
Pdf version : The rise of the s-Process in the Galaxy, ApJ, 617, 1091 (2004).
Pdf version : HST Observations of Heavy Elements in Metal-Poor Galactic Halo Stars, astro-ph/0502591, Astrophys. J., 627, 238 (2005).
Pdf version : Neutron-Capture Element Abundances in Halo Stars, astro-ph/0409552, in ASP Conf. Ser., Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis ed. T. Barnes and F. Bash (San Francisco: ASP), 313 (2005).
Pdf version : Near-UV Observations of CS2947-030: New Constraints on Neutron-Capture Nucleosynthesis Processes, astro-ph/0505002, Astrophys. J., 627, L145 (2005).
Pdf version : Improved Laboratory Transition Probabilities for Pt I and Application to the Platiunum Abundances of BD +17 3248 and the Sun, Astrophys. J., 619, 639 (2005).
Pdf version : Sm Transition Probabilities and Abundances,'' astro-ph/0510585, Astrophys. J. Supp., 162, 227 (2006).
Pdf version : Near-UV Observations of HD221170: New Insights into the Nature of r-Process-Rich Stars, astro-ph/0604180, Astrophys. J., 645, 613 (2006).
Pdf version : Nucleosynthesis: Stellar and Solar Abundances and Atomic Data, astro-ph/0605137, in the Proceedings of the NASA Laboratory Astrophysics Workshop (2006).
Pdf version : Gd Transition Probabilities and Abundances, astro-ph/0609487, Astrohys. J. Supp., 167, 292 (2006).
Pdf version : In Memory of Al Cameron, arXiv:astro-ph/0611824, http://indico.cern.ch/conferenceTimeTable.py?confId=059, in Nuclei in the Cosmos-IX, 205 (2006)
Pdf version : r-Process Enhanced Halo Stars, arXiv:astro-ph/0610412, http://indico.cern.ch/conferenceTimeTable. py?confId=059, in Nuclei in the Cosmos-IX, 14 (2006)
Pdf version : Hf Transition Probabilities and Abundances, astro-ph/0611036, Astrophys. J. Supp., 169, 120 (2007).
Pdf version : Explorations of the r-Processes: Comparisons between Calculations and Observations of Low-Metallicity Stars, astro-ph/0703091, Astrophys. J., 662, 39 (2007).
Pdf version : Nucleosynthesis in the Early Galaxy, Astrophys. J., 671, 1685 (2007).
Pdf version : Abundance Signatures in Halo Stars, in First Stars III (2008)
Pdf version : Nucleosynthesis Modes in the High-Entropy-Wind Scenario of Type II Supernovae, in First Stars III (2008)
Pdf version : Europium, Samarium, and Neodymium Isotopic Fractions in Metal-Poor Stars, in First Stars III (2008)
Pdf version : Europium, Samarium and Neodymium Isotopic Fractions in Metal-Poor Stars, astro-ph/0712.2473, Astrophys. J., 675, 723 (2008).
Pdf version : The Hobby-Eberly Telescope "Chemical Abundances of Stars in the Halo" (CASH) Project. I. The Lithium-, s-, and r-Enhanced Metal-Poor Giant HKII 17435-00532, arXiv:0802.3701, Astrophys. J., 679, 1549 (2008).
Pdf version : Er II Transition Probabilities and Abundances arXiv:0804.4465, Astrophys. J. Supp., in press (2008).
Postscript manuscript with color figures: Probing the Neutron-Capture Nucleosynthesis History of the Early Galaxy astro-ph/0209308, PASP, 114, 1293 (2002).
Pdf journal version with black and white figures: Probing the Neutron-Capture Nucleosynthesis History of the Early Galaxy astro-ph/0209308, PASP, 114, 1293 (2002).
Pdf manuscript with color figures: The Genesis of the Heaviest Elements in the Milky Way Galaxy Science, 299, 70 (2003).
Pdf manuscript with color figures: Advances in r-Process Nucleosynthesis in Carnegie Observatories Astrophysics Series, Vol. 4: Origin and Evolution of the Elements, ed. A. McWilliam & M. Rauch (Cambridge: Cambridge Univ. Press), 27 (2004)
Pdf manuscript with color figures: R-Process Nucleosynthesis in Supernovae Physics Today, Volume 57 Number 10, 47 (October, 2004). Copyright (2004) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. Website link to Physics Today
Pdf manuscript with color figures: Heavy Element Synthesis in the Oldest Stars and the Early Universe Nature, Volume 440, 1151 (April 27, 2006). This article may be downloaded for personal use only. Any other use requires prior permission of the author and Nature Publishing Group. Website link to Nature
Pdf article: Journal Club: An astronomer invites you to contemplate the history of the some of the oldest stars in the Universe. Nature, Volume 440, 129 (January 11, 2007). This article may be downloaded for personal use only. Any other use requires prior permission of the author and Nature Publishing Group. Website link to Nature
Pdf article: Essay in Concepts: A Constant Surprise Nature, Volume 448, 29 (July 5, 2007). This article may be downloaded for personal use only. Any other use requires prior permission of the author and Nature Publishing Group. Website link to Nature
Nuclear Astrophysics 12: ``Halo Star Abundances and Heavy Element Nucleosynthesis''
STAN Meeting 2004 :
FIRST STARS AND THE EVOLUTION OF THE UNIVERSE Meeting 2006 :
The talk at First Stars and the Evolution of the Universe
VISTARS 2005 pics:
More Vistars pics:
A trip to Saltzburg, Austria:
People and places in Saltzburg
A trip to FKT's farmhouse, France:
VISTARS 2006 pics:
NIC 2006 pics:
FRANZ and GERMANY pics:
Talk at the FRANZ meeting -- PDF version of power point talk: ``Neutron Capture Elements in Ultra-Metal-Poor Stars,''
Blois and France pics:
Talk at the blois meeting -- PDF version of power point talk: ``The r-Process in Halo Stars,''
Poster at First Stars III -- PDF version : ``Abundance Signatures in Halo Stars: Clues to Nucleosynthesis in the First Stars,''
Pdf version of power point talk: ``Probing the Nucleosynthesis Producst of the First Stars,'' Meeting on the Chemical Enrichment of the Early Universe, Santa Fe, NM (2004).
Pdf version of power point talk: ``Stellar Abundance Observations and the R-Process,'' JINA Workshop on the Discussion of the R-Process, Notre Dame, IN (2005).
Working hard at the JINA meeting:
Pdf version of power point talk: ``R-Process Signatures in Halo Stars, '' 2nd Vistars Workshop, Russbach, Austria (2005).
Pdf version of power point talk: ``Stellar Abundance Observations and Heavy Element Formation, '' AAS Meeting, Minneapolis, MN (2005).
Pdf version of power point talk: ``The Age of the Oldest Stars as a Constraint on Cosmological Models,'' Meeting on Outstanding Questions for the Standard Cosmological Model, London, England (2007).
1. The first image shows actual stellar spectra taken with the Hubble Space Telescope, HST. (The data are transmitted from the satellite to the computers at the Space Telescope Science Institute and then sent over the Internet 2 to our computers here at OU.) The spectral lines are in the ultraviolet portion of the spectra and are not visible on the ground - only space telescopes, like the HST are capable of such observations. These observations are the first to ever detect gold (Au) in old stars, thousands of light years from earth.
HST SPECTRA OF STARS IN THE GALACTIC HALO
2. Abundance observations - note elements such as Barium (Ba), Europium (Eu), and the radioactive element Thorium (Th) - of the star CS 22892-052, which is one of the oldest stars in the universe and located approximately 6,000 light years away. The observations were obtained using both ground-based (Keck and McDonald) and Space-Based (HST) Telescopes:
ABUNDANCES IN CS 22892--052, ONE OF THE OLDEST STARS IN THE UNIVERSE
Images of galaxies taken with the Radio Telescopes of the Very Large Array (VLA) near Socorro, New Mexico:
3. Galaxy NGC 7331, located approximately 30 million light
years away, appears to contain a
Massive Black Hole. This black hole was detected by researchers here
at OU (see ``Discovery of a Nuclear X-ray
Source in NGC 7331:'') A GALAXY
WITH A MASSIVE BLACK HOLE
-- A GALAXY
WITH A MASSIVE BLACK HOLE (jpeg format)
4. Galaxy M83, located approximately 20 million light years away, contains
a number of exploding stars
known as supernovae. These include supernovae 1957D, 1950B and 1923A
still radiating in the radio,
and detected by OU researchers, almost 80 years after it exploded.
A GALAXY
WITH A NUMBER OF SUPERNOVAE OR EXPLODING STARS
MY RESEARCH INTERESTS: A BRIEF DESCRIPTION
CURRICULUM VITA: PUBLICATIONS, ETC.
MY ACTIVITIES AT THE UNIVERSITY OF OKLAHOMA: TEACHING, ADVISING, ETC.
Radio FITS DATA 6 CM FITS file for G25.5.
Radio FITS DATA 20 CM FITS file for M83.
Radio FITS DATA 20 CM FITS file for NGC 7331.
Radio FITS DATA 6 CM FITS file for NGC 7331.
London (2007) at the Conference on Outstanding Questions for the Standard Cosmological Model
The boys at CES in Vegas (Venetian)
Linda's trip to Bellagio in 2006
Mom and Meg and Family pictures
Carmen Pantoja and JC at the Washington AAS meeting in January of 2006
Last Updated 06/20/08