JINA - Virtual Journal of Nuclear Astrophysics, 12 May 2006
Volume 4, Issue 19 (36 Articles)
- # 1 - A Large Stellar Evolution Database for Population Synthesis Studies. II. Stellar Models and Isochrones for an α-enhanced Metal Distribution
- # 2 - A Possible Approach to Three-dimensional Cosmic-Ray Propagation in the Galaxy. II. Stable Nuclei with Energy Change
- # 3 - The Dwarf Novae during Quiescence
- # 4 - Hydrodynamic Simulations of He Shell Flash Convection
- Astrophysical Journal - Volume 642, Issue 2 - May, 2006
- ABSTRACT, FULL TEXT WITH ENHANCEMENTS, PDF (3488 kB), PS
- # 5 - Neutron-Capture Elements in the s- and r-Process-rich Stars: Constraints on Neutron-Capture Nucleosynthesis Processes
- # 6 - Permitted Oxygen Abundances and the Temperature Scale of Metal-poor Turnoff Stars
- Astrophysical Journal - Volume 642, Issue 2 - May, 2006
- ABSTRACT, FULL TEXT WITH ENHANCEMENTS, PDF (482 kB), PS
- # 7 - Gamma-Ray Bursts
- # 8 - The X-ray Halo of GX5-1
- # 9 - Oscillator Strengths and Predissociation Rates for Rydberg Transitions in 12C16O, 13C16O, and 13C18O Involving the E 1Pi, B 1Sigma+, and W 1Pi States
- # 10 - Abundances of s-process elements in planetary nebulae: Br, Kr & Xe
- # 11 - Why the cosmological constant is small and positive
- # 12 - Topical Review on "Beta-beams"
- # 13 - Theoretical Aspects of High Energy Neutrinos and GRB
- # 14 - The Birth of Quark Stars: Photon-driven Supernovae?
- # 15 - The First Jet in the Universe: Protostellar Jets from the First Stars
- # 16 - Nucleosynthesis: Stellar and Solar Abundances and Atomic Data
- # 17 - Relativistic mechanics of neutron superfluid in (magneto) elastic star crust
- # 18 - Supernova Neutrinos: The Accretion Disk Scenario
- # 19 - Energy Injection in GRB Afterglow Models
- # 20 - $^6$Li Production by the Radiative Decay of Long-Lived Particles
- # 21 - The First Extrasolar Planet Discovered with a New Generation High Throughput Doppler Instrument
- # 22 - Carbon stars in local group dwarf galaxies: C and O abundances
- # 23 - Big Bang Nucleosynthesis Constraints on Hadronically and Electromagnetically Decaying Relic Particles
- # 24 - C+O detonations in thermonuclear supernovae: Interaction with previously burned material
- # 25 - The chemical compositions of the extreme halo stars HE0107-5240 and HE1327-2326 inferred from 3D hydrodynamical model atmospheres
- # 26 - Compilation of Giant Electric Dipole Resonances Built on Excited States
- # 27 - On the evolution of the symmetry energy of hot neutron-rich matter formed in heavy-ion reactions
- # 28 - Anisotropic thermal emission from magnetized neutron stars
- Astronomy and Astrophysics - Volume 451, Issue 3 - May, 2006
- Abstract, Full HTML, PDF file (1.98 MB), PS file (830 KB), References
- # 29 - Protoneutron star dynamos: pulsars, magnetars, and radio-silent X-ray emitting neutron stars
- Astronomy and Astrophysics - Volume 451, Issue 3 - May, 2006
- Abstract, Full HTML, PDF file (100 KB), PS file (45.8 KB), References
- # 30 - Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
- Astronomy and Astrophysics - Volume 451, Issue 3 - May, 2006
- Abstract, Full HTML, PDF file (420 KB), PS file (199 KB), References
- # 31 - Probing cosmic chemical evolution with gamma-ray bursts: GRB 060206 at z = 4.048
- Astronomy and Astrophysics - Volume 451, Issue 3 - May, 2006
- Abstract, Full HTML, PDF file (211 KB), PS file (256 KB), References
- # 32 - Reconstructing Supernova-Neutrino Spectra using Low-Energy Beta Beams
- Physics Review Letters - Vol.96, Issue 17 - 2 May 2006
- 172301 Abstract Full Text: [ PDF (307 kB) GZipped PS ]
- # 33 - Constraints on Cosmic Neutrino Fluxes from the Antarctic Impulsive Transient Antenna Experiment
- Physics Review Letters - Vol.96, Issue 17 - 4 May 2006
- 171101 Abstract Full Text: [ PDF (231 kB) GZipped PS ]
- # 34 - NASA BUDGET: Crisis Deepens as Scientists Fail to Rejigger Space Research
- # 35 - SCHOLARLY PUBLISHING: Bill Would Require Free Public Access to Research Papers
- # 36 - ASTRONOMY: A Hawaiian Upstart Prepares to Monitor the Starry Heavens
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.