JINA - Segue Virtual Journal, 15 November 2013
Volume 8, Issue 46 (12 Articles)
- # 1 - A spectroscopic binary in the Hercules dwarf spheroidal galaxy
- arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
- arXiv:1311.2582 [pdf, ps, other]
- # 2 - Atmospheric Parameters and Metallicities for 2191 stars in the Globular Cluster M4
- arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
- arXiv:1311.2592 [pdf, ps, other]
- # 3 - Atomic data for S II - Toward Better Diagnostics of Chemical Evolution in High-redshift Galaxies
- arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
- arXiv:1311.2553 [pdf, other]
- # 4 - H0 Revisited
- arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
- arXiv:1311.3461 [pdf, other]
- # 5 - NGC 1817, NGC 2141, and Berkeley 81: three BOCCE clusters of intermediate age
- arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
- arXiv:1311.2469 [pdf, ps, other]
- # 6 - On the metallicity of open clusters II. Spectroscopy
- arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
- arXiv:1311.2306 [pdf, other]
- # 7 - PyWiFeS: A Rapid Data Reduction Pipeline for the Wide Field Spectrograph (WiFeS)
- arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
- arXiv:1311.2666 [pdf, other]
- # 8 - Terzan 8: a Sagittarius-flavoured globular cluster
- arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Nov
- arXiv:1311.2589 [pdf, ps, other]
- # 9 - Hint of Dark Matter May Be Just Cosmic Ray Debris
- Science - Volume: 342, Issue: 6160
- # 10 - What's So Special About Science (And How Much Should We Spend on It?)
- Science - Volume: 342, Issue: 6160
- # 11 - Exploring the Chemical Link between Local Ellipticals and Their High-redshift Progenitors
- The Astrophysical Journal Letters - Volume: 778, Issue: 2
- View article PDF (885 KB)
- # 12 - What is the Difference? Blazhko and Non-Blazhko RRab Stars and the Special Case of V123 in M3
- The Astrophysical Journal Letters - Volume: 778, Issue: 2
- View article PDF (2.44 MB)
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.

