Results 1 to 10 of about 1,210,183 (255)

Nebular abundances of southern symbiotic stars [PDF]

open access: yes, 2005
We have calculated relative elemental abundances for a sample of 43 symbiotic stars. Helium abundances and the relative elemental abundances N/O, Ne/O, Ar/O were derived from new spectra collected in the optical range through low dispersion spectroscopy.
Almog   +33 more
arxiv   +3 more sources

Non-LTE Abundances of Magnesium, Aluminum and Sulfur in OB Stars Near the Solar Circle [PDF]

open access: yesAstron.Astrophys. 399 (2003) 525-530, 2002
Non-LTE abundances of magnesium, aluminum and sulfur are derived for a sample of 23 low-v \sin i stars belonging to six northern OB associations of the Galactic disk within 1 kpc of the Sun. The abundances are obtained from the fitting of synthetic line profiles to high resolution spectra.
Afflerbach   +21 more
arxiv   +5 more sources

Constraining solar abundances using helioseismology [PDF]

open access: yesAstrophys.J. 606 (2004) L85, 2004
Recent analyses of solar photospheric abundances suggest that the oxygen abundance in the solar atmosphere needs to be revised downwards. In this study we investigate the consequence of this revision on helioseismic analyses of the depth of the solar convection zone and the helium abundance in the solar envelope and find no significant effect.
Antia, H. M., Basu, Sarbani
arxiv   +5 more sources

Solar and stellar photospheric abundances

open access: yesLiving Reviews in Solar Physics, 2016
The determination of photospheric abundances in late-type stars from spectroscopic observations is a well-established field, built on solid theoretical foundations.
Carlos Allende Prieto
doaj   +4 more sources

The Interaction Between Accretion from the Interstellar Medium and Accretion from the Evolved Binary Component in Barium Stars [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2018
The reanalysis of the previously published abundance pattern of mild barium star HD202109 (ζ Cyg) and the chemical compositions of 129 thin disk barium stars facilitated the search for possible correlations of different stellar parameters with second ...
Yeuncheol Jeong   +2 more
doaj   +1 more source

MODELING MICROBIAL ABUNDANCES AND DYSBIOSIS WITH BETA-BINOMIAL REGRESSION. [PDF]

open access: yesAnnals of Applied Statistics, 2019
Using a sample from a population to estimate the proportion of the population with a certain category label is a broadly important problem. In the context of microbiome studies, this problem arises when researchers wish to use a sample from a population ...
Bryan D. Martin, D. Witten, A. Willis
semanticscholar   +1 more source

Mass–Metallicity Trends in Transiting Exoplanets from Atmospheric Abundances of H2O, Na, and K [PDF]

open access: yesAstrophysical Journal, 2019
Atmospheric compositions can provide powerful diagnostics of formation and migration histories of planetary systems. We investigate constraints on atmospheric abundances of H2O, Na, and K, in a sample of transiting exoplanets using the latest ...
L. Welbanks   +5 more
semanticscholar   +1 more source

Retrieving Temperatures and Abundances of Exoplanet Atmospheres with High-resolution Cross-correlation Spectroscopy [PDF]

open access: yesAstronomical Journal, 2018
High-resolution spectroscopy (R ≥ 25,000) has recently emerged as one of the leading methods for detecting atomic and molecular species in the atmospheres of exoplanets.
M. Brogi, M. Line
semanticscholar   +1 more source

Meta-analysis reveals declines in terrestrial but increases in freshwater insect abundances

open access: yesScience, 2020
Local drivers of decline matter Recent studies have reported alarming declines in insect populations, but questions persist about the breadth and pattern of such declines. van Klink et al.
Roel van Klink   +5 more
semanticscholar   +1 more source

Elemental and molecular abundances in comet 67P/Churyumov-Gerasimenko [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
Comets are considered to be some of the most pristine and unprocessed Solar system objects accessible to in situ exploration. Investigating their molecular and elemental composition takes us on a journey back to the early period of our Solar system and
M. Rubin   +20 more
semanticscholar   +1 more source

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