JINA - Segue Virtual Journal,
23 February 2018
Volume 13, Issue 8 (18 Articles)
- # 1 - Galaxies, Globular Clusters, and Dark Matter
- # 2 - Stellar Model Chromospheres and Spectroscopic Diagnostics
- # 3 - Neutron Star Mergers and Nucleosynthesis of Heavy Elements
- # 4 - Global survey of star clusters in the Milky Way VI. Age distribution and cluster formation history. (arXiv:1802.06779v1 [astro-ph.GA])
- # 5 - Impacts of nuclear-physics uncertainties in the s-process determined by Monte-Carlo variations. (arXiv:1802.05836v1 [astro-ph.SR])
- # 6 - Observing multiple populations in globular clusters with the ESO archive: NGC 6388 reloaded. (arXiv:1802.06787v1 [astro-ph.SR])
- Eugenio Carretta (1), Angela Bragaglia (1) ((1) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna)
- http://arxiv.org/abs/1802.06787
- # 7 - Precise Ages of Field Stars from White Dwarf Companions. (arXiv:1802.06663v1 [astro-ph.SR])
- # 8 - Progenitors of Core-Collapse Supernovae. (arXiv:1802.07503v1 [astro-ph.SR])
- # 9 - Sensitivity to neutron captures and beta-decays of the enhanced s-process in rotating massive stars at low metallicities. (arXiv:1802.05837v1 [astro-ph.SR])
- # 10 - The chemical connection between Damped Lyman-$alpha$ systems and Local Group dwarf galaxies. (arXiv:1802.07325v1 [astro-ph.GA])
- # 11 - The Galactic Thick Disc density profile traced with RR Lyrae stars. (arXiv:1802.07798v1 [astro-ph.GA])
- # 12 - The local rotation curve of the Milky Way based on SEGUE and RAVE data. (arXiv:1802.07658v1 [astro-ph.GA])
- K. Sysoliatina (1), A. Just (1), O. Golubov (2,3,4), Q.A. Parker (5,6), E.K. Grebel (1), G. Kordopatis (17), T. Zwitter (15), J. Bland-Hawthorn (14), B.K. Gibson (8), A. Kunder (16), U. Munari (7), J. Navarro (12), W. Reid (10,11), G. Seabroke (9), M.Steinmetz (18), F. Watson (13) ((1) Astronomisches Rechen-Institut, Heidelberg, Germany, (2) Schools of Physics, Technology, Karazin Kharkiv National University, Kharkiv, Ukraine, (3) Institute of Astronomy, Karazin Kharkiv National University, Kharkiv, Ukraine, (4) Department of Aerospace Engineering Sciences, University of Colorado at Boulder, USA, (5) Department of Physics, the University of Hong Kong, China, (6) The Laboratory for Space Research, the university of Hong Kong, China, (7) INAF Astronomical Observatory of Padova, Italy, (8) E.A. Milne Centre for Astrophysics, University of Hull, UK, (9) Mullard Space Science Laboratory, University College London, UK, (10) Department of Physics, Astronomy, Macquarie University, Sydney, Australia, (11) Western Sydney University, Australia, (12) Senior CIfAR Fellow, University of Victoria, Canada, (13) Australian Astronomical Observatory (14) Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia, (15) Faculty of Mathematics, Physics, University of Ljubljana, Slovenia, (16) Saint Martin's University, Lacey, USA, (17) Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, France, (18) Leibniz Institut für Astrophysik Potsdam, Germany)
- http://arxiv.org/abs/1802.07658
- # 13 - The selection function of the LAMOST Spectroscopic Survey of the Galactic Anticentre. (arXiv:1802.06777v1 [astro-ph.GA])
- # 14 - The Updated BaSTI Stellar Evolution Models and Isochrones: I. Solar Scaled Calculations. (arXiv:1802.07319v1 [astro-ph.GA])
- S. L. Hidalgo (1, 2), A. Pietrinferni (3), S. Cassisi (3), M. Salaris (4), A. Mucciarelli (5, 6), A. Savino (4, 7), A. Aparicio (1, 2), V. Silva Aguirre (8), K. Verma (8) ((1) Instituto de Astrofísica de Canarias, (2) Department of Astrophysics of University of La Laguna, (3) INAF-Osservatorio Astronomico d'Abruzzo, (4) Astrophysics Research Institute Liverpool John Moores University, (5) Dipartimento di Fisica e Astronomia - Universitá a degli Studi di Bologna, (6) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, (7) Kapteyn Astronomical Institute University of Groningen, (8) Stellar Astrophysics Centre Department of Physics, Astronomy Aarhus University)
- http://arxiv.org/abs/1802.07319
- # 15 - The World Space Observatory Ultraviolet (WSO-UV), as a bridge to future UV astronomy. (arXiv:1802.06849v1 [astro-ph.IM])
- # 16 - Chemical Abundances in the Leading Arm of the Magellanic Stream
- Andrew J. Fox, Kathleen A. Barger, Bart P. Wakker, Philipp Richter, Jacqueline Antwi-Danso, Dana I. Casetti-Dinescu, J. Christopher Howk, Nicolas Lehner, Elena DâOnghia, Paul A. Crowther,, Felix J. Lockman
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/854/2/142
- # 17 - Near-infrared Stellar Populations in the Metal-poor, Dwarf Irregular Galaxies Sextans A and Leo A
- # 18 - Stellar Multiplicity Meets Stellar Evolution and Metallicity: The APOGEE View
- Carles Badenes, Christine Mazzola, Todd A. Thompson, Kevin Covey, Peter E. Freeman, Matthew G. Walker, Maxwell Moe, Nicholas Troup, David Nidever, Carlos Allende Prieto, Brett Andrews, Rodolfo H. Barbá, Timothy C. Beers, Jo Bovy, Joleen K. Carlberg, Nathan De Lee, Jennifer Johnson, Hannah Lewis, Steven R. Majewski, Marc Pinsonneault, Jennifer Sobeck, Keivan G. Stassun, Guy S. Stringfellow,, Gail Zasowski
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/854/2/147
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.