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词条 Swan band
释义

  1. See also

  2. References

Swan bands are a characteristic of the spectra of carbon stars, comets and of burning hydrocarbon fuels.[1][2] They are named for the Scottish physicist William Swan, who first studied the spectral analysis of radical diatomic carbon (C2) in 1856.[3]

Swan bands consist of several sequences of vibrational bands scattered throughout the visible spectrum.[4]

See also

  • Spectroscopy

References

1. ^{{cite journal |author=R.C. Johnson |date=1927 |title=The structure and origin of the Swan band spectrum of carbon |journal=Philosophical Transactions of the Royal Society A |volume=226 |pages=157–230 |doi=10.1098/rsta.1927.0005 |bibcode = 1927RSPTA.226..157J |issue=636–646 |url=http://rsta.royalsocietypublishing.org/content/roypta/226/636-646/157.full.pdf }}
2. ^{{cite journal |author=W.E. Pretty |date=1927 |title=The Swan band spectrum of carbon |journal=Proceedings of the Physical Society |volume=40 |pages=71–78 |doi=10.1088/0959-5309/40/1/313|bibcode = 1927PPS....40...71P }}
3. ^{{cite journal |author=W. Swan |date=1857 |title=On the prismatic spectra of the flames of compounds of carbon and hydrogen |journal=Transactions of the Royal Society of Edinburgh |volume=21 |pages=411–430 |url = https://books.google.com/books?id=GHAxAQAAMAAJ&pg=PA411#v=onepage&q&f=false}}
4. ^{{cite journal |author=Robert B. King |date=1948 |title= Relative Transition Probabilities of the Swan Bands of Carbon |journal=Astrophysical Journal |volume=108 |pages=429 |bibcode = 1948ApJ...108..429K |doi = 10.1086/145078 }}
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