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- W3205732200 abstract "The wavelength dependence of polarization of 21 polarized stars near the Orion Nebula has been measured. Most stars fit the standard interstellar law. The wavelength of maximum linear polarization, lambda/sub max/, ranges from normal values to 0.71..mu..m. The polarimetric, spectroscopic, and photometric data support a normal reddening law (Rapprox. =3) for most Orion stars, and present evidence for unusually large grain sizes in front of some Orion stars. For the stars BR 545 and BR 885 large values of lambda/sub max/ are associated with unusually large values of total to selective extinction.A division of the observed polarization into intracluster dust and circumstellar shell components shows that the presence of shells does not usually lead to linear polarization in the optical wavelength region. Also, no association of polarization with known light variability could be found. The nature of the intracluster dust clouds is discussed briefly.The results of searches for circular polarization as well as short-period variability are presented in two appendices." @default.
- W3205732200 created "2021-10-25" @default.
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- W3205732200 date "1976-09-01" @default.
- W3205732200 modified "2023-09-24" @default.
- W3205732200 title "Intracluster Dust, Circumstellar Shells and the Wavelength Dependence of Polarization in Orion." @default.
- W3205732200 hasPublicationYear "1976" @default.
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