Showing 1–20 of 62 results
/ Date/ Name
Jul 28, 2009Statistical equilibrium of silicon in the atmospheres of metal-poor starsJun 29, 2015The early days of the Sculptor dwarf spheroidal galaxyJul 21, 2014The Hamburg/ESO R-process Enhanced Star survey (HERES) X. HE 2252-4225, one more r-process enhanced and actinide-boost halo starMar 12, 2012A primordial star in the heart of the LionApr 7, 2015Calibrating the α parameter of convective efficiency using observed stellar propertiesJul 14, 2017Influence of inelastic collisions with hydrogen atoms on the non-LTE modelling of Ca I and Ca II lines in late-type starsNov 19, 2015Accuracy of atmospheric parameters of FGK dwarfs determined by spectrum fittingNov 28, 2007Non-LTE line formation for heavy elements in four very metal-poor starsJan 24, 2011A non-LTE study of neutral and singly-ionized iron line spectra in 1D models of the Sun and selected late-type starsJan 19, 2023BD+30$^\circ$549: young helium-weak silicon star in NGC 1333 star-forming regionNov 21, 2008Non-LTE line formation for Pr II and Pr III in A and Ap starsNov 14, 2023Influence of departures from LTE on determinations of the scandium abundances in A-B type starsOct 1, 2016Systematic non-LTE study of the $-2.6 \le$ [Fe/H] $\le 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to EuAug 21, 2004The Hamburg/ESO R-process Enhanced Star survey (HERES). I. Project description, and discovery of two stars with strong enhancements of neutron-capture elementsFeb 1, 2011Formation of Zr I and II lines under non-LTE conditions of stellar atmospheresMar 18, 2010The Hamburg/ESO R-process Enhanced Star survey (HERES). V. Detailed abundance analysis of the r-process enhanced star HE 2327-5642Jul 10, 20231D non-LTE corrections for chemical abundance analyses of very metal-poor starsJun 15, 2022Detailed abundances of the wide pairs of stars with and without planets: the binary systems 16 Cyg and HD 219542Sep 14, 2017The formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis. II. Early chemical enrichmentJun 4, 2015Systematic NLTE study of the -2.6 < [Fe/H] < 0.2 F and G dwarfs in the solar neighbourhood. I. Stellar atmosphere parameters