Results 191 to 200 of about 5,740 (219)
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Astronomische Nachrichten, 2001
Original article can be found at: http://www3.interscience.wiley.com Copyright WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim [Full text of this article is not available in the UHRA]
H. Edelmann, U. Heber, R. Napiwotzki
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Original article can be found at: http://www3.interscience.wiley.com Copyright WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim [Full text of this article is not available in the UHRA]
H. Edelmann, U. Heber, R. Napiwotzki
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Vanadium abundances in early A stars
Publications of the Astronomical Society of the Pacific, 1978Vanadium-to-hydrogen ratios have been determined for Omicron Peg, HR 6127, HR 465 (rare-earth minimum), and HR 8216. With respect to the solar system, vanadium is overabundant in the first two stars, possibly normal in the third, and underabundant in the fourth.
C. R. Cowley +2 more
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On the use of sulphur as a tracer for abundances in galaxies
Monthly Notices of the Royal Astronomical Society, 2022Angeles Isabel Díaz Beltran +1 more
exaly
Star-to-star nitrogen abundances in globular cluster stars
Nuclear Physics A, 2001F. Grundahl, M. Briley
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Hot stars and cosmic abundances
2014Hot massive stars are ideal indicators for present-day cosmic abundances. We review results from a non-LTE study of a larger sample of early B-type stars in the solar neighbourhood by Nieva & Przybilla (2012) and extend the analysis. Using comprehensive models with improved microphysics, novel analysis methodologies and high-quality spectra it is shown
Przybilla, Norbert +3 more
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Abundance analysis of carbon stars
2003info:eu-repo/semantics ...
Masseron, Thomas +4 more
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Galactic simulations of r-process elemental abundances
Monthly Notices of the Royal Astronomical Society, 2019Chiaki Kobayashi
exaly
An empirical calibration of nebular abundances based on the sulphur emission lines
Monthly Notices of the Royal Astronomical Society, 2000Angeles Isabel Díaz Beltran +1 more
exaly

