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- Blanketing_effect abstract "The blanketing effect (also referred to as line blanketing or the line-blanketing effect) is the enhancement of the red or infrared regions of a stellar spectrum at the expense of the other regions, with an overall diminishing effect on the whole spectrum. The term originates in a 1928 article by astrophysicist Edward Arthur Milne, where it was used to describe the effects that the astronomical metals in a star's outer regions had on that star's spectrum. The name arose because the absorption lines act as a "blanket", causing the continuum temperature of the spectrum to rise over what it would have been if these lines were not present.Astronomical metals, which produce most of a star's spectral absorption lines, absorb a fraction of the star's radiant energy (a phenomenon known as the blocking effect) and then re-emit it at a lower frequency as part of the backwarming effect. The combination of both these effects results in the position of stars in a color-color diagram to shift towards redder areas as the proportion of metals in them increases. The blanketing effect is thus highly dependent on the metallicity index of a star, which indicates the fraction of elements other than hydrogen and helium that compose it.".
- Blanketing_effect wikiPageExternalLink 1969PASP...81..826M.
- Blanketing_effect wikiPageExternalLink books?id=L5zuAAAAMAAJ&hl=en&source=gbs_navlinks_s.
- Blanketing_effect wikiPageExternalLink c6.pdf.
- Blanketing_effect wikiPageExternalLink line-blanketing-astronomy.
- Blanketing_effect wikiPageExternalLink node7.html.
- Blanketing_effect wikiPageID "36197961".
- Blanketing_effect wikiPageLength "2844".
- Blanketing_effect wikiPageOutDegree "10".
- Blanketing_effect wikiPageRevisionID "680650121".
- Blanketing_effect wikiPageWikiLink Absorption_line.
- Blanketing_effect wikiPageWikiLink Astronomical_spectroscopy.
- Blanketing_effect wikiPageWikiLink Category:Astronomy.
- Blanketing_effect wikiPageWikiLink Color-color_diagram.
- Blanketing_effect wikiPageWikiLink Color–color_diagram.
- Blanketing_effect wikiPageWikiLink Edward_Arthur_Milne.
- Blanketing_effect wikiPageWikiLink Infrared.
- Blanketing_effect wikiPageWikiLink Metallicity.
- Blanketing_effect wikiPageWikiLink Radiant_energy.
- Blanketing_effect wikiPageWikiLink Red.
- Blanketing_effect wikiPageWikiLink Spectral_line.
- Blanketing_effect wikiPageWikiLink Stellar_spectrum.
- Blanketing_effect wikiPageWikiLinkText "Blanketing effect".
- Blanketing_effect hasPhotoCollection Blanketing_effect.
- Blanketing_effect wikiPageUsesTemplate Template:Reflist.
- Blanketing_effect subject Category:Astronomy.
- Blanketing_effect hypernym Enhancement.
- Blanketing_effect type Software.
- Blanketing_effect comment "The blanketing effect (also referred to as line blanketing or the line-blanketing effect) is the enhancement of the red or infrared regions of a stellar spectrum at the expense of the other regions, with an overall diminishing effect on the whole spectrum. The term originates in a 1928 article by astrophysicist Edward Arthur Milne, where it was used to describe the effects that the astronomical metals in a star's outer regions had on that star's spectrum.".
- Blanketing_effect label "Blanketing effect".
- Blanketing_effect sameAs m.0vpx04m.
- Blanketing_effect sameAs Q17005937.
- Blanketing_effect sameAs Q17005937.
- Blanketing_effect wasDerivedFrom Blanketing_effect?oldid=680650121.
- Blanketing_effect isPrimaryTopicOf Blanketing_effect.