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Unveiling the Active Nucleus of Centaurus A |
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1 week 1 day ago |
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Linear Polarization due to Lower Level Depopulation Pumping in Stellar Atmospheres |
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1 week 1 day ago |
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Non-LTE Inversion of Stokes Profiles Induced by the Zeeman Effect |
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1 week 1 day ago |
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Time Series of Solar Granulation Images. II. Evolution of Individual Granules |
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A search for delta Scuti stars in northern open clusters. I. CCD photometry of NGC 7245, NGC 7062, NGC 7226 and NGC 7654 |
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1 week 1 day ago |
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Seismology of delta Scuti stars in the Praesepe cluster. II. Identification of radial modes and their associated stellar parameters |
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Discovery of a Low-Mass Brown Dwarf Companion of the Young Nearby Star G 196-3 |
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A Search for Very Low Mass Stars and Brown Dwarfs in the Young sigma Orionis Cluster |
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Lithium and rotation in the Hyades late F and G stars |
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Distribution, sizes, and luminosity function of the HII regions in NGC 4321 |
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The striking near-infrared morphology of the inner region in M100 |
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The Central Region in M100: Observations and Modeling |
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Statistics and properties of H II regions in a sample of grand-design galaxies. II. Physical properties. |
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A New Chemo-evolutionary Population Synthesis Model for Early-Type Galaxies. I. Theoretical Basis |
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Internal turbulence, viriality, and density bounding of the most luminous H II regions in the spiral galaxy M 100 |
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Kinematics of Ionized and Molecular Hydrogen in the Core of M100 |
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The ionized gas in the spiral galaxy NGC 3359. II. Kinematics |
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Populations of High-Luminosity Density-bounded H II Regions in Spiral Galaxies: Evidence and Implications |
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Chaotic quantization of field theories |
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The Shape of the Luminosity Profiles of Bulges of Spiral Galaxies |
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Two Tails in NGC 3656 and the Major Merger Origin of Shell and Minor-Axis Dust Lane Elliptical Galaxies |
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A strong correlation between bar strength and global star forming activity in isolated barred galaxies |
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ASASSN-24fw: Candidate Gas-rich Circumsecondary Disk Occultation of a Main-sequence Star |
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1 week 6 days ago |
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How Accurately Can Obscured Galaxy Luminosities Be Measured Using Spectral Energy Distribution Fitting of Near- through Far-infrared Observations? |
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LiteBIRD science goals and forecasts. E-mode anomalies |
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