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Gasdynamics in NGC 5248: Fueling a Circumnuclear Starburst Ring of Super-Star Clusters |
iacweb |
6 months 2 weeks ago |
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Chemical analysis of 8 recently discovered extra-solar planet host stars |
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6 months 2 weeks ago |
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Sulphur Abundance in Very Metal-poor Stars |
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6 months 2 weeks ago |
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On the Period-Luminosity-Colour-Metallicity relation and the pulsational characteristics of lambda Bootis type stars |
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6 months 2 weeks ago |
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Spatially resolved spectroscopy of WR ring nebulae. III - New results and chemical properties of the sample |
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6 months 2 weeks ago |
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EXPORT: Spectral classification and projected rotational velocities of Vega-type and pre-main sequence stars |
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6 months 2 weeks ago |
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The orbital period of the recurrent X-ray transient in Terzan 6 |
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6 months 2 weeks ago |
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Observation of Convective Collapse and Upward-moving Shocks in the Quiet Sun |
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An ellipsoidal modulation in X-ray Nova VELA 1993 (=GRS 1009-45) |
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The mass ratio of Nova MUSCAE 1991 |
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The mass of X-ray Nova Scorpii1994 (=GRO J1655-40) |
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Hα flares from V404 Cyg in quiescence |
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The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy |
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6 months 2 weeks ago |
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Fabry-Perot observations of the ionized gas in the spiral galaxy NGC 6951 |
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6 months 2 weeks ago |
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Detailed analysis of Balmer lines in cool dwarf stars |
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6 months 2 weeks ago |
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On the chlorine abundance in H II regions |
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7 months 1 week ago |
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Hyperspectral imaging of meteorites using the HyperScout-H instrument |
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7 months 1 week ago |
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Correction to: Trio of super-Earth candidates orbiting K-dwarf HD 48948: a new habitable zone candidate |
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Spectroscopy and asteroseismic modelling of the red giant binary system KIC 10841730 |
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Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 b |
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Strong lithium lines in red supergiants at different metallicities |
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Are early-type galaxies quenched by present-day environment?: A study of dwarfs in the Fornax Cluster |
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Magnetic Fields beneath Active Region Coronal Loops |
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LSPE-Strip on-sky calibration strategy using bright celestial sources |
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The two rings of (50000) Quaoar (Corrigendum) |
iacweb |
7 months 1 week ago |
