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Matches in DBpedia 2016-04 for { <http://dbpedia.org/resource/Struve–Sahade_effect> ?p ?o }

• Struve–Sahade_effect abstract "The Struve–Sahade effect (S–S effect) occurs with a double-lined spectroscopic binary star system. A spectroscopic binary is called double-lined when the absorption lines of both stars can be observed with a spectroscope. As each member of the star system approaches the observer in turn, the absorption lines of that star are shifted toward the blue end of the optical spectrum by the Doppler effect. Likewise, as a star moves away, its lines are shifted toward the red end of the spectrum. Each of these absorption lines has a characteristic strength that depends on the physical properties of the photosphere. The Struve–Sahade effect occurs when these lines become anomalously weaker as a star's spectrum is red-shifted.This effect was first reported by Otto Struve in 1937. It became important because the effect called into question the values of parameters such as mass and luminosity ratios in massive spectroscopic binary systems. In 1950, Struve attempted to explain the effect as the result of streams of gas trailing behind the secondary star, causing the star to be obscured when the star was moving away. In 1959, Jorge Sahade produced a model where a gaseous stream extended from the primary to the secondary member of the binary, and the opacity of this stream produced the weakening of the absorption lines. The effect then became known as the Struve–Sahade effect. In 1997, Gies and colleagues provided an alternative explanation, arguing that the collision between the stellar winds from the two stars results in a bow shock that is deflected by the Coriolis force, placing it in an obscuring position along the line of sight to the secondary star. Other hypotheses have since been created to explain this effect.".
• Struve–Sahade_effect wikiPageID "30642120".
• Struve–Sahade_effect wikiPageLength "3290".
• Struve–Sahade_effect wikiPageOutDegree "11".
• Struve–Sahade_effect wikiPageRevisionID "654441688".
• Struve–Sahade_effect wikiPageWikiLink Binary_star.
• Struve–Sahade_effect wikiPageWikiLink Category:Binary_stars.
• Struve–Sahade_effect wikiPageWikiLink Category:Emission_spectroscopy.
• Struve–Sahade_effect wikiPageWikiLink Colliding-wind_binary.
• Struve–Sahade_effect wikiPageWikiLink Coriolis_force.
• Struve–Sahade_effect wikiPageWikiLink Doppler_effect.
• Struve–Sahade_effect wikiPageWikiLink Jorge_Sahade.
• Struve–Sahade_effect wikiPageWikiLink Optical_spectrometer.
• Struve–Sahade_effect wikiPageWikiLink Otto_Struve.
• Struve–Sahade_effect wikiPageWikiLink Photosphere.
• Struve–Sahade_effect wikiPageWikiLink Spectral_line.
• Struve–Sahade_effect wikiPageWikiLinkText "Struve–Sahade effect".
• Struve–Sahade_effect wikiPageUsesTemplate Template:Astronomy-stub.
• Struve–Sahade_effect wikiPageUsesTemplate Template:Reflist.
• Struve–Sahade_effect subject Category:Binary_stars.
• Struve–Sahade_effect subject Category:Emission_spectroscopy.
• Struve–Sahade_effect type Physic.
• Struve–Sahade_effect type Redirect.
• Struve–Sahade_effect comment "The Struve–Sahade effect (S–S effect) occurs with a double-lined spectroscopic binary star system. A spectroscopic binary is called double-lined when the absorption lines of both stars can be observed with a spectroscope. As each member of the star system approaches the observer in turn, the absorption lines of that star are shifted toward the blue end of the optical spectrum by the Doppler effect. Likewise, as a star moves away, its lines are shifted toward the red end of the spectrum.".
• Struve–Sahade_effect label "Struve–Sahade effect".
• Struve–Sahade_effect sameAs Q3720184.
• Struve–Sahade_effect sameAs Struve-Sahade-Effekt.
• Struve–Sahade_effect sameAs Effetto_Struve-Sahade.
• Struve–Sahade_effect sameAs m.0g9tz5f.
• Struve–Sahade_effect sameAs Q3720184.
• Struve–Sahade_effect wasDerivedFrom Struve–Sahade_effect?oldid=654441688.
• Struve–Sahade_effect isPrimaryTopicOf Struve–Sahade_effect.