JINA - Segue Virtual Journal, 17 August 2012
Volume 7, Issue 33 (34 Articles)
- # 1 - A new gravitational N-body simulation algorithm for investigation of cosmological chaotic advection
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.3444 [pdf, other]
- # 2 - Absolute Magnitude Calibration for Red Giants based on the Colour-Magnitude Diagrams of Galactic Clusters. III-Calibration with 2MASS
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.3196 [pdf, ps, other]
- # 3 - Bayesian astrostatistics: a backward look to the future
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.3036 [pdf, ps, other]
- # 4 - Binary Evolution Leads to Two Populations of White Dwarf Companions
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.2276 [pdf, other]
- # 5 - Data challenges of time domain astronomy
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.2480 [pdf, ps, other]
- # 6 - Metal-poor Galaxies in the Local Universe
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.2894 [pdf, ps, other]
- # 7 - On the future of astrostatistics: statistical foundations and statistical practice
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.3035 [pdf, ps, other]
- # 8 - Radial velocities for the Hipparcos-Gaia Hundred-Thousand-Proper-Motion project
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.3048 [pdf, other]
- # 9 - Satellites and Haloes of Dwarf Galaxies
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.2027 [pdf, ps, other]
- # 10 - Stellar Diameters and Temperatures II. Main Sequence K & M Stars
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.2431 [pdf, ps, other]
- # 11 - The Absolute Magnitude of RRc Variables From Statistical Parallax
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.2689 [pdf, other]
- # 12 - The Most Metal-Poor Stars. I. Discovery, Data, and Atmospheric Parameters
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.2999 [pdf, ps, other]
- # 13 - The Most Metal-Poor Stars. II. Chemical Abundances of 190 Metal-Poor Stars Including 10 New Stars With [Fe/H] < -3.5
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.3003 [pdf, ps, other]
- # 14 - The Most Metal-Poor Stars. III. The Metallicity Distribution Function and CEMP Fraction
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.3016 [pdf, ps, other]
- # 15 - The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey
- arXiv.org - Astrophysics - Volume: 2012, Issue: 17 Aug
- arXiv:1208.2233 [pdf, other]
- # 16 - Heterogeneity of the population of open star clusters in the Galaxy
- Astronomy Letters - Volume: 38, Issue: 8
- Download PDF (784.3 KB)
- # 17 - Two populations of open star clusters in the Galaxy
- Astronomy Letters - Volume: 38, Issue: 8
- Download PDF (865.0 KB)
- # 18 - Cosmology: Enigma at the heart of the Universe
- Nature - Volume: 488, Issue: 7411
- 253-424
- # 19 - The search for a primordial magnetic field
- Physics Reports - Volume: 517, Issue: 5
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PDF (1419 K) | Related articles | Related reference work articles
- # 20 - Big or Small, Science Will Suffer If Sequestration Goes Into Effect
- Science - Volume: 337, Issue: 6096
- # 21 - Detection of a Second-generation Binary in the Globular Cluster ω Centauri
- The Astrophysical Journal - Volume: 755, Issue: 1
- Abstract References Full text PDF (444 KB) View as HTML
- # 22 - Models for Metal-poor Stars with Enhanced Abundances of C, N, O, Ne, Na, Mg, Si, S, Ca, and Ti, in Turn, at Constant Helium and Iron Abundances
- The Astrophysical Journal - Volume: 755, Issue: 1
- Abstract References Full text PDF (1.43 MB) View as HTML
- # 23 - The Importance of Disk Structure in Stalling Type I Migration
- The Astrophysical Journal - Volume: 755, Issue: 1
- Abstract References Full text PDF (1.07 MB) View as HTML
- # 24 - The Source Density and Observability of Pair-instability Supernovae from the First Stars
- The Astrophysical Journal - Volume: 755, Issue: 1
- Abstract References Full text PDF (2.06 MB) View as HTML
- # 25 - Tracing the Origin of the Aquarius Stream. I
- The Astrophysical Journal - Volume: 755, Issue: 1
- Abstract References Full text PDF (470 KB) View as HTML
- # 26 - HIP 38939B: A New Benchmark T Dwarf in the Galactic Plane Discovered with Pan-STARRS1
- The Astrophysical Journal - Volume: 755, Issue: 2
- Abstract References Full text PDF (796 KB) View as HTML
- # 27 - Metallicity Evolution of Damped Lyα Systems Out to z ~ 5
- The Astrophysical Journal - Volume: 755, Issue: 2
- Abstract References Full text PDF (5.49 MB) HTML with Enhancements
- # 28 - The Vertical Motions of Mono-abundance Sub-populations in the Milky Way Disk
- The Astrophysical Journal - Volume: 755, Issue: 2
- Abstract References Full text PDF (1.75 MB) View as HTML
- # 29 - Two Distant Halo Velocity Groups Discovered by the Palomar Transient Factory
- The Astrophysical Journal - Volume: 755, Issue: 2
- Abstract References Full text PDF (574 KB) View as HTML
- # 30 - A New CEMP-s RR Lyrae Star
- The Astrophysical Journal Letters - Volume: 755, Issue: 1
- Abstract References Full text PDF (216 KB) View as HTML
- # 31 - Building the Stellar Halo through Feedback in Dwarf Galaxies
- The Astrophysical Journal Letters - Volume: 755, Issue: 2
- Abstract References Full text PDF (314 KB) View as HTML
- # 32 - Dark Matter, Magnetic Fields, and the Rotation Curve of the Milky Way
- The Astrophysical Journal Letters - Volume: 755, Issue: 2
- Abstract References Full text PDF (208 KB) View as HTML
- # 33 - High-resolution Reddening Map in the Direction of the Stellar System Terzan 5
- The Astrophysical Journal Letters - Volume: 755, Issue: 2
- Abstract References Full text PDF (6.96 MB) View as HTML
- # 34 - The Apache Point Observatory Galactic Evolution Experiment: First Detection of High-velocity Milky Way Bar Stars
- The Astrophysical Journal Letters - Volume: 755, Issue: 2
- Abstract References Full text PDF (791 KB) View as HTML
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.

