The metal–poor end of the Spite plateau: gravity sensitivity of the Hα wings fitting.

By L. Sbordone, P. Bonifacio, E. Caffau, H. Ludwig, N. Behara, Jonay I. Gonzalez-Hernandez, M. Steffen, R. Cayrel, Bernd Freytag, C. V. Veer and 9 more. Proceedings of the International Astronomical Union, 2009

360 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/f762e7fcb19cabb41db5f9489f3bc65422949324

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In Astronomy and Astrophysics

1. C. Steidel
2. M. Pettini
3. A. Shapley
4. B. Famaey
5. Naveen A. Reddy
6. D. Erb
7. P. Hopkins
8. A. Frebel

In Instrumentation

1. C. Steidel
2. M. Pettini
3. A. Shapley
4. B. Famaey
5. Naveen A. Reddy
6. D. Erb
7. A. Frebel
8. J. Norris

In Statistical and Nonlinear Physics

1. B. Famaey
2. C. Steidel
3. J. Norris
4. S. McGaugh
5. A. Frebel
6. M. Pettini
7. P. Hopkins
8. Mikhail Ivanov

Citations in the corpus

• Near-Field Cosmology with Extremely Metal-Poor Stars (2015, background): “…Thorburn (1994), Ryan, Norris & Beers (1999), Charbonnel & Primas (2005), Asplund et al. (2006), Bonifacio et al. (2007), Aoki et al. (2009b), Meléndez et al. (2010), Sbordone et al. (2010), Bonifacio et al. (2012b), and references therein, for details of some of the observational contributions.”
• Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions (2011, result): “It has been suggested that turbulent mixing might result in the depletion of primordial lithium necessary to reconcile lithium with the CMB (upward pointing arrow [287]), while others [405] argue that this would merely reconcile some discrepant stars with the bulk of the data defining the Spite plat”
• One Percent Determination of the Primordial Deuterium Abundance (2017, background): “…in metal-poor star forming galaxies (Izotov, Thuan, & Guseva 2014; Aver, Olive, & Skillman 2015),1 while the primordial 7Li abundance is determined from the atmospheres of very metal-poor stars (Asplund et al. 2006; Aoki et al. 2009; Meléndez et al. 2010; Sbordone et al. 2010; Spite et al. 2015).”
• A new, precise measurement of the primordial abundance of deuterium (2012, background): “On the other hand, a satisfactory explanation for the factor of ∼ 3 discrepancy between the abundances of 7Li in the oldest stars in our Galaxy and the value expected from BBN has yet to be found (Sbordone et al. 2010; Iocco 2012; Nissen & Schuster 2012 and references therein).”
• STANDARD BIG BANG NUCLEOSYNTHESIS UP TO CNO WITH AN IMPROVED EXTENDED NUCLEAR NETWORK (2011, neutral): “A more recent analysis by Sbordone et al. (2010) gives Li/H = (1.58 ± 0.31) × 10−10.”