JINA - Segue Virtual Journal, 14 January 2011
Volume 6, Issue 2 (14 Articles)
- # 1 - A Deep Photometric Look at Two of Andromeda's Dwarf Spheroidals: X and XVII
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2201 [pdf, ps, other]
- # 2 - An Optical-UV Survey of the North Celestial Cap
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.1604 [pdf, ps, other]
- # 3 - Chemically tagging the Hyades stream: Does it partly originate from the Hyades cluster?
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2583 [pdf, ps, other]
- # 4 - Constraining the orbital history of the Magellanic Clouds: A new bound scenario suggested by the tidal origin of the Magellanic Stream
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2500 [pdf, other]
- # 5 - First stars XIII. Two extremely metal-poor RR Lyrae stars?
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2207 [pdf, ps, other]
- # 6 - Galaxy Disks
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.1771 [pdf, other]
- # 7 - How Does Feedback Affect Milky Way Satellite Formation?
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2232 [pdf, other]
- # 8 - Nucleosynthesis and gamma-ray lines
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2112 [pdf, ps, other]
- # 9 - Sagittarius and its siblings in the Aquarius simulations
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2544 [pdf, ps, other]
- # 10 - The Ancient Globular Clusters Were Much More Massive At Birth
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2208 [pdf, ps, other]
- # 11 - The M33 Globular Cluster System with PAndAS Data: The Last Outer Halo Cluster?
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2450 [pdf, ps, other]
- # 12 - Topics on Galactic Chemical Evolution
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2108 [pdf, ps, other]
- # 13 - [O/Fe] Estimates for Carbon-Enhanced Metal-Poor Stars from Near-IR Spectroscopy
- arXiv.org - Astrophysics - Volume: 2011, Issue: 14 Jan
- arXiv:1101.2260 [pdf, ps, other]
- # 14 - An Evolving Stellar Initial Mass Function and the Gamma-ray Burst Redshift Distribution
- The Astrophysical Journal Letters - Volume: 727, Issue: 2
- Abstract References Full text PDF (274 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.

