Sean G. Ryan mostly deals with Astrophysics, Stars, Astronomy, Nucleosynthesis and Metallicity. His Spectral line research extends to Astrophysics, which is thematically connected. The study incorporates disciplines such as Spectroscopy, Supernova and Equivalent width in addition to Stars.
He does research in Astronomy, focusing on Milky Way specifically. His Nucleosynthesis course of study focuses on Subgiant and Stellar mass, Giant star, Stellar nucleosynthesis, Star formation and K-type main-sequence star. The concepts of his Metallicity study are interwoven with issues in Halo and Galaxy formation and evolution.
Sean G. Ryan mainly focuses on Astrophysics, Stars, Astronomy, Nucleosynthesis and Metallicity. In general Astrophysics study, his work on Galaxy, Galactic halo and Halo often relates to the realm of Population, thereby connecting several areas of interest. Sean G. Ryan works mostly in the field of Galaxy, limiting it down to topics relating to Equivalent width and, in certain cases, Diffuse interstellar band.
Within one scientific family, Sean G. Ryan focuses on topics pertaining to Supernova under Stars, and may sometimes address concerns connected to Cosmic ray. His research in Nucleosynthesis intersects with topics in Subgiant, Abundance of the chemical elements and Radial velocity. His studies in Spectral line integrate themes in fields like Line and Atomic physics.
Sean G. Ryan spends much of his time researching Astrophysics, Stars, Nucleosynthesis, Astronomy and Galaxy. Sean G. Ryan performs multidisciplinary study in Astrophysics and Population in his work. In the field of Stars, his study on Metallicity and Stellar atmosphere overlaps with subjects such as Metal.
His Nucleosynthesis research incorporates themes from Spectral line, Abundance of the chemical elements and Spectroscopy. His research on Astronomy often connects related areas such as Neutron capture. In general Galaxy, his work in Halo, Quasar and Diffuse interstellar band is often linked to Thermodynamic equilibrium and Organic molecules linking many areas of study.
Sean G. Ryan mainly investigates Astrophysics, Stars, Nucleosynthesis, Astronomy and Abundance of the chemical elements. His studies link Spectrograph with Astrophysics. His Stars study incorporates themes from William Herschel Telescope and Wavelength range.
His Nucleosynthesis study integrates concerns from other disciplines, such as Spectroscopy, Spectral line, Stellar atmosphere, Subgiant and Star. His work in Milky Way and Galactic halo is related to Astronomy. In his work, Giant star is strongly intertwined with Stellar evolution, which is a subfield of Abundance of the chemical elements.
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The Gaia-ESO Public Spectroscopic Survey
G. Gilmore;S. Randich;M. Asplund;J. Binney.
The Messenger (2012)
Extremely Metal-Poor Stars. II. Elemental Abundances and the Early Chemical Enrichment of The Galaxy*
Sean G. Ryan;John E. Norris;Timothy C. Beers.
The Astrophysical Journal (1996)
Nucleosynthetic signatures of the first stars
Anna Frebel;Wako Aoki;Norbert Christlieb;Hiroyasu Ando.
Nature (2005)
Carbon-enhanced Metal-poor Stars. I. Chemical Compositions of 26 Stars*
Wako Aoki;Timothy C. Beers;Norbert Christlieb;John E. Norris.
The Astrophysical Journal (2007)
Primordial Lithium and Big Bang Nucleosynthesis.
Sean G. Ryan;Timothy C. Beers;Keith A. Olive;Brian D. Fields.
The Astrophysical Journal (2000)
The Spite Lithium Plateau: Ultrathin but Postprimordial
Sean G. Ryan;John E. Norris;Timothy C. Beers.
The Astrophysical Journal (1999)
The Spite Lithium Plateau: Ultra-Thin but Post-Primordial
Sean G. Ryan;John E. Norris;Timothy C. Beers.
arXiv: Astrophysics (1999)
EXTREMELY METAL-POOR STARS. VIII. HIGH-RESOLUTION, HIGH SIGNAL-TO-NOISE RATIO ANALYSIS OF FIVE STARS WITH (Fe/H) ( (3.5
John E. Norris;Sean G. Ryan;Timothy C. Beers.
The Astrophysical Journal (2001)
The Binary Frequency Among Carbon-enhanced, s-Process-rich, Metal-poor Stars
Sara Lucatello;Sara Lucatello;Stelios Tsangarides;Timothy C. Beers;Eugenio Carretta.
The Astrophysical Journal (2005)
Extremely Metal-Poor Stars. VIII. High-Resolution, High-Signal-To-Noise Analysis of Five Stars with [Fe/H] < -3.5
John E. Norris;Sean G. Ryan;Timothy C. Beers.
arXiv: Astrophysics (2001)
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