โญ ๐๐๐ฌ๐ญ๐ฌ๐๐ฅ๐ฅ๐๐ซ ๐๐ฅ๐๐ซ๐ญ: ๐๐๐ง๐ค๐๐ #๐ ๐ข๐ง ๐๐ก๐ฒ๐ฌ๐ข๐๐ฌ ๐จ๐ ๐๐ญ๐๐ญ๐ข๐๐ฌ ๐จ๐ง ๐๐ฆ๐๐ณ๐จ๐ง!
๐ผ๐จ๐ฉ๐ง๐ค๐ฃ๐ค๐ข๐๐๐๐ก ๐๐ฅ๐๐๐ฉ๐ง๐ค๐จ๐๐ค๐ฅ๐ฎ (๐๐ง๐ ๐๐๐๐ฉ๐๐ค๐ฃ) by ๐๐จ๐ง๐๐ญ๐ก๐๐ง ๐๐๐ง๐ง๐ฒ๐ฌ๐จ๐ง (
@ucl, UK) is your step-by-step guide to understanding the physics behind astronomical spectra.
From the hydrogen atom to small molecules, this edition uses actual astronomical spectra to illustrate the theory and show what information can be retrieved from light emitted by stars, nebulae, and other celestial objects. Comprehensive exercises, with answers, make it ideal for ๐ฎ๐ง๐๐๐ซ๐ ๐ซ๐๐๐ฎ๐๐ญ๐๐ฌ, ๐ฉ๐จ๐ฌ๐ญ๐ ๐ซ๐๐๐ฎ๐๐ญ๐๐ฌ, ๐๐ง๐ ๐ซ๐๐ฌ๐๐๐ซ๐๐ก๐๐ซ๐ฌ seeking hands-on understanding of atomic and molecular spectroscopy.
๐ก ๐๐๐ฒ ๐
๐๐๐ญ๐ฎ๐ซ๐๐ฌ:
โช๏ธ Comprehensive introduction to atomic and molecular physics in astronomy
โช๏ธ Real spectra used to connect theory to observation
โช๏ธ Exercises with solutions to reinforce learning
๐ ๐๐ฑ๐ฉ๐ฅ๐จ๐ซ๐ ๐ญ๐ก๐ ๐๐จ๐จ๐ค ๐ก๐๐ซ๐:
doi.org/10.1142/q0207
๐๐ฆ๐๐ณ๐จ๐ง:
us.amazon.com/Astronomical-Sโฆ
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