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Technetium-rich M stars: Prime diagnostics of recent third dredge-up events on the asymptotic giant branch |
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Investigating Phosphorus Abundances in a Sample of APOGEE-2 Bulge Globular Clusters |
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Solvent-Free Solid State Dechlorination of C 60 Cl 6 and C 60 Cl 12 with Cesium Iodide |
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Structures and Properties of Fan-Shaped Jets: Hα Dark Blobs and Transparent Regions |
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Roadmap on carbon molecular nanostructures in space |
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Deep survey of millimeter radio recombination lines toward the planetary nebulae IC 418 and NGC 7027 |
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High energy radiation induced degradation of poly(lactic acid) (PLLA) film: radiation chemical yield, kinetics, mechanism and radioracemization evidences |
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Hexa-(2-ethylhexyl)-hexa-peri-hexabenzocoronene as archetypal model compound of asphaltenes and MAONs |
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A comprehensive Gaia view of ellipsoidal and rotational red giant binaries |
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On the Metallicity of Star-forming Dwarf Galaxies |
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Evolutionary synthesis models of starbursts. IV. Soft X-ray emission |
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Keck Spectroscopy of Globular Clusters in the Sombrero Galaxy |
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The spatial distribution of coalescing neutron star binaries: implications for gamma-ray bursts |
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GTC telescope mechanics design |
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Propagation experiments in the near infrared along a 150-km path and from stars in the Canarian archipelago |
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The quasar fraction in low-frequency-selected complete samples and implications for unified schemes |
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The Host Galaxy of the Lensed Quasar Q0957+561 |
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Star-forming Objects in the Tidal Tails of Compact Groups |
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On faint companions in the close environment of star-forming dwarf galaxies. Possible external star formation triggers? |
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Cusped Mass Models of Gravitational Lenses |
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Evolution of active galactic nuclei broad-line region clouds: low- and high-ionization lines |
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The Evolution of a Mass-selected Sample of Early-Type Field Galaxies |
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SN 1988A in M58 - A type II-P supernova with a high late-time luminosity |
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The response of the broad emission line region to ionizing continuum variations. III - an atlas of transfer functions |
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On the massive star-forming capacity of molecular clouds |
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