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 ⓘ
Harvard astronomy program ⓘ
author Cecilia Payne-Gaposchkin ⓘ
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 ⓘ