Where, oh where has the r-process gone?

[1]  T. Beers,et al.  Carbon-enhanced Metal-poor Stars: Osmium and Iridium Abundances in the Neutron-Capture-enhanced Subgiants CS 31062-050 and LP 625-44 , 2006, astro-ph/0609138.

[2]  I. Ivans,et al.  Near-Ultraviolet Observations of HD 221170: New Insights into the Nature of r-Process-rich Stars , 2006, astro-ph/0604180.

[3]  S. Ryan,et al.  Neutron-Capture Elements in the Very Metal Poor Star HD 122563 , 2006, astro-ph/0602107.

[4]  Hamburg,et al.  The Hamburg/ESO R-process enhanced star survey (HERES) - III. HE 0338-3945 and the formation of the r + s stars , 2006, astro-ph/0601476.

[5]  G. Wasserburg,et al.  Metal Enrichment of the Intergalactic Medium and Production of Massive Black Holes , 2005, astro-ph/0509151.

[6]  L. Ho,et al.  Measuring Stellar Velocity Dispersions in Active Galaxies , 2005, astro-ph/0512462.

[7]  S. Wanajo,et al.  R-process calculations and galactic chemical evolution , 2005, astro-ph/0511518.

[8]  T. Beers,et al.  Enrichment of Very Metal Poor Stars with Both r-Process and s-Process Elements from 8-10 M☉ Stars , 2005, astro-ph/0509788.

[9]  F. Herwig.  Evolution of Asymptotic Giant Branch Stars , 2005 .

[10]  K. Nomoto,et al.  The First Chemical Enrichment in the Universe and the Formation of Hyper Metal-Poor Stars , 2005, Science.

[11]  T. Beers,et al.  Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements , 2005, astro-ph/0503032.

[12]  T. Beers,et al.  Nucleosynthetic signatures of the first stars , 2005, Nature.

[13]  M. Bichler,et al.  New half-life measurement of 182Hf: improved chronometer for the early solar system. , 2004, Physical review letters.

[14]  R. Michael Rich,et al.  Draco 119: A Remarkable Heavy-Element-deficient Giant , 2004, astro-ph/0409646.

[15]  E. Tolstoy,et al.  Stellar Chemical Signatures and Hierarchical Galaxy Formation , 2004, astro-ph/0406120.

[16]  Jennifer A. Johnson,et al.  The s-Process in Metal-Poor Stars: Abundances for 22 Neutron-Capture Elements in CS 31062-050 , 2004, astro-ph/0402003.

[17]  C. Sneden,et al.  # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. GALACTIC EVOLUTION OF Sr, Y, AND Zr: A MULTIPLICITY OF NUCLEOSYNTHETIC PROCESSES , 2003 .

[18]  D. Argast,et al.  Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early Galaxy , 2003, astro-ph/0309237.

[19]  C. Sneden,et al.  Binary Blue Metal-poor Stars: Evidence for Asymptotic Giant Branch Mass Transfer , 2003, astro-ph/0304064.

[20]  V. Hill,et al.  The Extremely Metal-poor, Neutron Capture-rich Star CS 22892-052: A Comprehensive Abundance Analysis , 2003, astro-ph/0303542.

[21]  T. Beers,et al.  The r-Process in Supernova Explosions from the Collapse of O-Ne-Mg Cores , 2003, astro-ph/0302261.

[22]  G. Wasserburg,et al.  Abundance Analysis of HE 2148–1247, A Star with Extremely Enhanced Neutron Capture Elements , 2003, astro-ph/0301460.

[23]  G. Wasserburg,et al.  Stellar Sources for Heavy r-Process Nuclei , 2003, astro-ph/0301461.

[24]  T. Beers,et al.  A stellar relic from the early Milky Way , 2002, Nature.

[25]  K. Mezger,et al.  Rapid accretion and early core formation on asteroids and the terrestrial planets from Hf–W chronometry , 2002, Nature.

[26]  F. Albarède,et al.  A short timescale for terrestrial planet formation from Hf–W chronometry of meteorites , 2002, Nature.

[27]  Jennifer A. Johnson,et al.  The r-Process in the Early Galaxy , 2002, astro-ph/0208375.

[28]  T. Beers,et al.  First stars. I. The extreme r-element rich, iron-poor halo giant CS 31082-001 - Implications for the r-process site(s) and radioactive cosmochronology , 2002, astro-ph/0203462.

[29]  T. Beers,et al.  The Chemical Composition and Age of the Metal-poor Halo Star BD +17°3248 , 2002, astro-ph/0202429.

[30]  G. Wasserburg,et al.  Determination of Nucleosynthetic Yields of Supernovae and Very Massive Stars from Abundances in Metal-Poor Stars , 2001, astro-ph/0110532.

[31]  A. Jorissen,et al.  Discovery of three lead-rich stars , 2001, Nature.

[32]  G. Wasserburg,et al.  A Model for Abundances in Metal-poor Stars , 2001, astro-ph/0106085.

[33]  A. Burrows,et al.  The Physics of Proto-Neutron Star Winds: Implications for r-Process Nucleosynthesis , 2001, astro-ph/0105004.

[34]  T. Beers,et al.  Measurement of stellar age from uranium decay , 2001, Nature.

[35]  C. Sneden,et al.  The r-Process-enriched Low-Metallicity Giant HD 115444 , 1999, astro-ph/9910376.

[36]  G. Wasserburg,et al.  Nucleosynthesis in asymptotic giant branch stars: Relevance for galactic enrichment and solar system formation , 1999 .

[37]  M. Busso,et al.  Neutron Capture in Low-Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures , 1999, astro-ph/9906266.

[38]  K. Kratz,et al.  The Astrophysical r-Process: A Comparison of Calculations following Adiabatic Expansion with Classical Calculations Based on Neutron Densities and Temperatures , 1999 .

[39]  E. García–Berro,et al.  On the Evolution of Stars that Form Electron-degenerate Cores Processed by Carbon Burning. V. Shell Convection Sustained by Helium Burning, Transient Neon Burning, Dredge-out, Urca Cooling, and Other Properties of an 11 M☉ Population I Model Star , 1999 .

[40]  F. Ferrini,et al.  Galactic Chemical Evolution of Heavy Elements: From Barium to Europium , 1999, astro-ph/9903451.

[41]  C. Sneden,et al.  Detection of Silver in Metal-poor Stars , 1998 .

[42]  A. Chieffi,et al.  Evolution and Nucleosynthesis in Low-Mass Asymptotic Giant Branch Stars. II. Neutron Capture and the s-Process , 1998 .

[43]  E. García–Berro,et al.  On the Evolution of Stars that Form Electron-degenerate Cores Processed by Carbon Burning. IV. Outward Mixing During the Second Dredge-up Phase and Other Properties of a 10.5 M☉ Model Star , 1997 .

[44]  B. Meyer,et al.  Survey of r-Process Models , 1997 .

[45]  Enrique García-Berro,et al.  On the Evolution of Stars that Form Electron-Degenerate Cores Processed by Carbon Burning. III. The Inward Propagation of a Carbon-Burning Flame and Other Properties of a 9 M☉ Model Star , 1997 .

[46]  M. Steinmetz,et al.  Energy Input and Mass Redistribution by Supernovae in the Interstellar Medium , 1997, astro-ph/9706175.

[47]  G. Wasserburg,et al.  Diverse Supernova Sources for the r-Process , 1997, astro-ph/9706120.

[48]  S. Woosley,et al.  Nucleosynthesis in Neutrino-driven Winds. II. Implications for Heavy Element Synthesis , 1996, astro-ph/9611097.

[49]  S. Woosley,et al.  Nucleosynthesis in Neutrino-Driven Winds. I. The Physical Conditions , 1996, astro-ph/9611094.

[50]  G. Preston,et al.  The Ultra--Metal-poor, Neutron-Capture--rich Giant Star CS 22892-052 , 1996 .

[51]  S. Jacobsen,et al.  Evidence for 182Hf in the early Solar System and constraints on the timescale of terrestrial accretion and core formation , 1996 .

[52]  D. Arnett,et al.  Supernovae and Nucleosynthesis , 1996 .

[53]  Enrique García-Berro,et al.  On the Evolution of Stars That Form Electron-degenerate Cores Processed by Carbon Burning. II. Isotope Abundances and Thermal Pulses in a 10 M sun Model with an ONe Core and Applications to Long-Period Variables, Classical Novae, and Accretion-induced Collapse , 1996 .

[54]  A. Halliday,et al.  Hafnium–tungsten chronometry and the timing of terrestrial core formation , 1995, Nature.

[55]  S. Woosley,et al.  The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis , 1995 .

[56]  I. Iben,et al.  On the formation and evolution of super-asymptotic giant branch stars with cores processed by carbon burning. 1: SPICA to Antares , 1994 .

[57]  James R. Wilson,et al.  The r-process and neutrino-heated supernova ejecta , 1994 .

[58]  K. Takahashi,et al.  Nucleosynthesis in neutrino-driven winds from protoneutron stars II. The r-process , 1994 .

[59]  G. Wasserburg,et al.  ASYMPTOTIC GIANT BRANCH STARS AS A SOURCE OF SHORT-LIVED RADIOACTIVE NUCLEI IN THE SOLAR NEBULA , 1994 .

[60]  W. M. Howard,et al.  Neutron-rich α-rich freeze-out and the r-process in the high-entropy neutrino-energized supernova bubble , 1993 .

[61]  Mathews,et al.  Connection between flavor-mixing of cosmologically significant neutrinos and heavy element nucleosynthesis in supernovae. , 1993, Physical review letters.

[62]  W. M. Howard,et al.  r-process nucleosynthesis in the high-entropy supernova bubble , 1992 .

[63]  S. Woosley,et al.  The alpha -Process and the r-Process , 1992 .

[64]  J. Cowan,et al.  Evolution of heavy-element abundances as a constraint on sites for neutron-capture nucleosynthesis , 1992 .

[65]  S. Woosley,et al.  The collapse of white dwarfs to neutron stars , 1992 .

[66]  S. Wood,et al.  Geochim. cosmochim. acta , 1990 .

[67]  C. Raiteri,et al.  S-Process Nucleosynthesis: Classical Approach and Asymptotic Giant Branch Models for Low-Mass Stars , 1990 .

[68]  K. Nomoto.  Evolution of 8--10 M sun Stars toward Electron Capture Supernovae. II. Collapse of an O + NE + MG Core , 1987 .

[69]  T. Beers,et al.  A Search for Stars of Very Low Metal Abundance. III. UBV Photometry of Metal-weak Candidates , 1985 .

[70]  James R. Wilson,et al.  Revival of a stalled supernova shock by neutrino heating , 1985 .

[71]  K. Nomoto.  Evolution of 8-10 solar mass stars toward electron capture supernovae. I - Formation of electron-degenerate O + NE + MG cores. , 1984 .

[72]  P. A. Seeger,et al.  Nucleosynthesis of Heavy Elements by Neutron Capture , 1965 .

[73]  F. Hoyle,et al.  Synthesis of the Elements in Stars , 1957 .

[74]  T. Beers,et al.  The Hamburg / ESO R-process Enhanced Star survey ( HERES ) ⋆ ⋆ ⋆ II . Spectroscopic analysis of the survey sample , 2008 .

[75]  T. Beers,et al.  The Hamburg / ESO R-process Enhanced Star survey ( HERES ) ⋆ I . Project description , and discovery of two stars with stro ng enhancements of neutron-capture elements , 2008 .

[76]  N. Grevesse,et al.  In: Origin and Evolution of the elements , 1993 .

[77]  Michel Casse,et al.  Origin and evolution of the elements , 1993 .

[78]  F. Thielemann,et al.  Isotopic r-process abundances and nuclear structure far from stability. , 1993 .

[79]  A. Wolfe,et al.  The redshift distribution of Ly-alpha clouds and the proximity effect , 1991 .

[80]  N. Grevesse,et al.  Abundances of the elements: Meteoritic and solar , 1989 .

[81]  S. Woosley,et al.  EVOLUTION AND EXPLOSION OF MASSIVE STARS * , 1978, Reviews of Modern Physics.

[82]  G. Wasserburg,et al.  Nucleochronologies and the Mean Age of the Elements , 1970 .