JINA - Segue Virtual Journal, 30 July 2010
Volume 5, Issue 31 (21 Articles)
- # 1 - A Complete Spectroscopic Survey of the Milky Way Satellite Segue 1: The Darkest Galaxy
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4198 [pdf, ps, other]
- # 2 - Abundances for a large sample of red giants in NGC 1851: hints for a merger of two clusters?
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.5301 [pdf, ps, other]
- # 3 - AstroGrid-D: Grid Technology for Astronomical Science
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4053 (cross-list from cs.DC) [pdf, other]
- # 4 - C, N and O abundances in red clump stars of the Milky Way
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4064 [pdf, ps, other]
- # 5 - CRIRES spectroscopy and empirical line-by-line identification of FeH molecular absorption in an M dwarf
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4116 [pdf, ps, other]
- # 6 - Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4411 [pdf, ps, other]
- # 7 - Indirect Dark Matter Detection Limits from the Ultra-Faint Milky Way Satellite Segue 1
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4199 [pdf, other]
- # 8 - Photometric characterization of the Galactic star cluster Trumpler 20
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4782 [pdf, ps, other]
- # 9 - Stratification of the elements in the atmospheres of blue horizontal-branch stars
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4023 [pdf, other]
- # 10 - The Use of Scientific Data: A Content Analysis
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4602 [pdf]
- # 11 - VLT Kinematics for omega Centauri: Further Support for a Central Black Hole
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4559 [pdf, ps, other]
- # 12 - X-shooter observations of main sequence stars in the globular cluster NGC 2808: first chemical tagging of a He-normal and a He-rich dwarf
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.5299 [pdf, ps, other]
- # 13 - A Correction to the Standard Galactic Reddening Map: Passive Galaxies as Standard Crayons
- The Astrophysical Journal - Volume: 719, Issue: 1
- Abstract References Full text PDF (2.40 MB) View as HTML
- # 14 - A New Galactic Extinction Map of the Cygnus Region
- The Astrophysical Journal - Volume: 719, Issue: 1
- Abstract References Full text PDF (7.31 MB) View as HTML
- # 15 - Cross Identification of Stars with Unknown Proper Motions
- The Astrophysical Journal - Volume: 719, Issue: 1
- Abstract References Full text PDF (500 KB) View as HTML
- # 16 - Monte Carlo Simulations of Globular Cluster Evolution. V. Binary Stellar Evolution
- The Astrophysical Journal - Volume: 719, Issue: 1
- Abstract References Full text PDF (2.30 MB) View as HTML
- # 17 - The Chemical Evolution of the Ursa Minor Dwarf Spheroidal Galaxy
- The Astrophysical Journal - Volume: 719, Issue: 1
- Abstract References Full text PDF (1.14 MB) HTML with Enhancements
- # 18 - The Evolution of Primordial Binary Open Star Clusters: Mergers, Shredded Secondaries, and Separated Twins
- The Astrophysical Journal - Volume: 719, Issue: 1
- Abstract References Full text PDF (3.16 MB) View as HTML
- # 19 - The Growth of Dark Matter Halos: Evidence for Significant Smooth Accretion
- The Astrophysical Journal - Volume: 719, Issue: 1
- Abstract References Full text PDF (1.50 MB) View as HTML
- # 20 - The Lick/SDSS Library. I. Synthetic Index Definition and Calibration
- The Astrophysical Journal - Volume: 719, Issue: 1
- Abstract References Full text PDF (8.54 MB) View as HTML
- # 21 - A Galactic Origin for HE 0437–5439, The Hypervelocity Star Near the Large Magellanic Cloud
- The Astrophysical Journal Letters - Volume: 719, Issue: 1
- Abstract References Full text PDF (581 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.

