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OverviewFull Product DetailsAuthor: A. Slettebak , A. SlettebakPublisher: Springer Imprint: Kluwer Academic Publishers Edition: 1976 ed. Volume: 70 Dimensions: Width: 17.00cm , Height: 2.50cm , Length: 24.40cm Weight: 0.900kg ISBN: 9789027707000ISBN 10: 9027707006 Pages: 465 Publication Date: 30 November 1976 Audience: Professional and scholarly , Professional & Vocational Format: Paperback Publisher's Status: Active Availability: Out of stock ![]() The supplier is temporarily out of stock of this item. It will be ordered for you on backorder and shipped when it becomes available. Table of ContentsIntroductory Address.- I/Observations of Be Stars.- Spectra and Photometry of Be Stars (Review Paper).- A Survey of H? in the Brighter, Northern Be Stars.- A Study of Be Stars in Clusters.- Emission Features of Several Be Stars as Related to their Luminosity Class and Spectral Type.- Rapid Variations in the Spectra of o And, ? Cas, and ? Oph.- Rapid Variations of H? in Be Stars.- Stellar Photometric Observations at H? through a Narrow-Band Interference Filter.- Spectroscopic Observations of Be Stars in the Near Infrared.- New Observational Data Concerning 4 Her and ? Tau.- The Surface Gravities of Be Stars.- A Comparative Study of the Shell of ? Tau and 48 Lib.- A Model for the Shell of HD 50138.- Observations Récentes de HD 200120.- Singly-Ionized Iron Emission Lines in the Spectra of Early Type Stars.- Pleione as a Variable Star.- Energy Distributions of Be Stars (Review Paper).- II/Be Stars as Rotating Stars.- Be Stars as Rotating Stars: Observations (Review Paper).- Ultraviolet Observations of Rapidly Rotating B-type Stars.- The Relationship of the Oe to the Be Stars.- H? and H? Measures as Related to Be Star Rotation.- III/ New Observational Techniques.- Radio Observations of Be Stars (Review Paper).- Ultraviolet Observations of Be Stars (Review Paper).- A Survey of Mass Loss from Be and Shell Stars, Using Ultraviolet Data from Copernicus.- Ultraviolet Si iv/C iv Ratios for Be Stars.- The Near Ultraviolet Spectrum of ? Tau.- Spectroscopic Observations of the Be Stars ? Cen, ? Cas, and ? Per.- The Far Ultraviolet Spectra of v Cyg and ? Cen.- Photographic Infrared Spectroscopy and Near Infrared Photometry of Be Stars (Review Paper).- Paschen Decrements in Be Stars.- The Classification of Faint Be Stars.- Polarization in Be Stars (Review Paper).-Polarization Measurements Across the Balmer Lines of Be and Shell Stars.- Intrinsic Linear Polarization of Be Stars as a Function of v sin i.- IV/Line Formation in Expanding Atmospheres.- Line Formation in Expanding Atmospheres (Review Paper).- Radiative Transfer in Dynamic Stellar Atmospheres.- Si II Lines in the Shell of ? Tau.- The Complex Structure of the Ca II H and K Lines in the Spectrum of the A0ep Star with Infrared Excess HD 190073.- Theoretical Emission-Line Profiles Computed at Ond?ejov.- Motions in the Shells and Atmospheres of V923 Aql and EW Lac and their Manifestation in the Spectrum.- V/Models.- Models for the Circumstellar Envelopes of Be Stars (Review Paper).- On the Possible Role of Magnetic Fields in the Dynamics of the Be Phenomenon.- Theoretical Wavelength Dependence of Polarization in Early-Type Stars.- The Possible Role of Radiative Acceleration in Supporting Extended Atmospheres in Be Stars.- VI /Single Versus Binary Stars.- Duplicity of Be Stars as Seen from Ond?ejov (Review Paper).- On the Detection of Binary Be Stars.- Evidence for the Existence of Mass-Exchange Binary Be Stars from Periodic Spectral Variations.- Toward a Model for the Be Binary System ? Per.- Final Remarks on the Binary Hypothesis for the Be Stars.- VII/ General Discussion.- General Discussion.- Concluding Remarks.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |