Microturbulence
![Arxiv:1709.05344V1 [Astro-Ph.SR] 15 Sep 2017 (A(Li) = 2.75), Higher Than Its Companion by 0.5 Dex](http://data.docslib.org/img/264x/095e450bac437441ae11460b37afaab0.webp)
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- DETAILED CHEMICAL ABUNDANCES in the Sgr and Cma DWARF GALAXIES
- The Rotation Rates of Massive Stars⋆
- Stellar Metallicities from Skymapper Photometry I: a Study of the Tucana II Ultra-Faint Dwarf Galaxy
- Measurements of Stellar Magnetic Fields Using Synthetic Spectrum Fitting
- Spectroscopic Determination of the Fundamental Parameters of 66 B
- THE TYPE Iib SUPERNOVA 2013Df and ITS COOL SUPERGIANT PROGENITOR
- Observational Constraints on the Origin of the Elements III
- Two Decades of Hypergiant Research
- Inferring the Composition of Super-Jupiter Mass Companions Of
- Physics of Eclipsing Binaries. Ii. Toward the Increased Model Fidelity A
- Microturbulence in O Supergiants
- (GIBS) II. Metallicity Distributions and Alpha Element Abundances at Fixed Galactic Latitude
- The Messenger
- Chemical and Kinematic Properties of Bright Metal Poor
- Eclipsing Binary Stars in Open Clusters
- The Rotation Rates of Massive Stars: How Slow Are the Slow Ones?
- Turbulence, Mass Loss and Hα Emission by Stochastic Shocks In
- Arxiv:1712.01297V1 [Astro-Ph.GA] 4 Dec 2017