Stellar Atmospheres

E576885

"Stellar Atmospheres" is a landmark astrophysics work that fundamentally advanced understanding of the physical properties and chemical composition of stars.

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Stellar Atmospheres canonical 1

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Predicate Object
instanceOf astrophysics book
book
scientific monograph
associatedWith Harvard College Observatory NERFINISHED
Harvard astronomy program
author Cecilia Payne-Gaposchkin NERFINISHED
contribution applied Saha ionization equation to stellar spectra
demonstrated that hydrogen is the most abundant element in stars
established that stellar spectral differences are mainly due to temperature, not composition
linked stellar spectral types to physical conditions in stellar atmospheres
showed that helium is highly abundant in stars
field astrophysics
stellar astrophysics
focusesOn chemical composition of stars
excitation in stellar atmospheres
ionization in stellar atmospheres
physical properties of stars
radiative transfer in stellar atmospheres
spectral line formation
genre non-fiction
scientific literature
hasImpactOn determination of elemental abundances in stars
interpretation of stellar spectra
understanding of the Sun’s composition
historicalSignificance challenged earlier assumptions about similarity of Sun and Earth composition
provided quantitative framework for stellar spectroscopy
influenced classification of stellar spectra
models of stellar structure and evolution
modern stellar astrophysics
language English
mainSubject stars
stellar atmospheres
stellar composition
stellar spectra
stellar structure
methodology application of atomic physics to stellar spectra
spectroscopic analysis
use of ionization equilibria in stellar atmospheres
notableFor being a landmark work in astrophysics
revolutionizing understanding of stellar composition
usedIn astronomy education
stellar atmosphere modeling

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Cecilia Payne-Gaposchkin notableWork Stellar Atmospheres