Monthly Archives: October 2016

The Opacity Project: computational methods

James Colgan Los Alamos National Laboratory, Los Alamos, NM 87545, USA This viewpoint relates to an article by K A Berrington et al (1987 J. Phys. B: At. Mol. Opt. Phys. 20 6379–97) and was published as part of a … Continue reading

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Systematic non-LTE study of the -2.6 < [Fe/H] < 0.2 F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu

Zhao, G.; Mashonkina, L.; Yan, H. L.; Alexeeva, S.; Kobayashi, C.; Pakhomov, Yu.; Shi, J. R.; Sitnova, T.; Tan, K. F.; Zhang, H. W.; Zhang, J. B.; Zhou, Z. M.; Bolte, M.; Chen, Y. Q.; Li, X.; Liu, F.; Zhai, … Continue reading

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3D NLTE analysis of the most iron-deficient star, SMSS0313-6708

Nordlander, Thomas; Amarsi, Anish M.; Lind, Karin; Asplund, Martin; Barklem, Paul S.; Casey, Andy R.; Collet, Remo; Leenaarts, Jorrit Models of star formation in the early universe depend on the details of accretion, fragmentation and radiative feedback. Different simulations predict … Continue reading

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