Results 221 to 230 of about 4,904 (241)
Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Veronig AM +12 more
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Tidal tail identification and detailed analysis of the open star cluster King 13 using Gaia DR3 and 2MASS. [PDF]
Ahmed NM, Darwish MS.
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A Faint Progenitor System for the Faint Supernova 2024vjm
Zimmerman E +69 more
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A binary merger product as the direct progenitor of a Type II-P supernova
Niu* Z +17 more
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V3101 Cyg: A Cataclysmic Variable Born with a Brown Dwarf Donor
Ramirez S +7 more
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Test of evolutionary models for stellar population studies
Journal of Astrophysics and Astronomy, 1994Using the Andersen (1991) data on the mass, absolute visual magnitude, the effective surface temperature and the bolometric corrections, new calibrations for the mass vs. absolute visual magnitude and for the bolometric correction vs. effective surface temperature have been derived.
N. Srivastva, R. K. Gulati, N. C. Rana
exaly +2 more sources
Stellar Evolutionary Models: current uncertainties
AIP Conference Proceedings, 2009In this last decade, our knowledge of evolutionary and structural properties of stars of different mass and chemical composition is significantly improved. This result has been achieved as a consequence of our improved capability in understanding and describing the physical behavior of stellar matter in the thermal regimes characteristic of the ...
Santi Cassisi +7 more
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AGB star atmospheres modeling as feedback to stellar evolutionary and galaxy models
Proceedings of the International Astronomical Union, 2018AbstractThe chemical enrichment of the Universe is considerably affected by the contribution of cool evolved stars. We studied the O-rich star R Peg and the C-rich star V Oph, using respectively the VLTI/GRAVITY and VLTI/MIDI instruments. We interpret the data using grids of 1-D and 3-D dynamic model atmospheres.
Gioia Rau +5 more
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An improved evolutionary model for stellar population applied to NGC 2903
Astrophysics and Space Science, 1990We outline the revised physical assumption which have been incorporated into our previously published evolutionary model for stellar population synthesis in galaxies. Applying the present version of the model to well-defined zones on the nucleus and along a spiral arm of NGC 2903 we show that the star formation rate has increased during the lifetime of
E. Casuso, J. E. Beckman, J. Cepa
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