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Author:   A. Slettebak
Publisher:   Springer
Imprint:   Kluwer Academic Publishers
Edition:   1976 ed.
Volume:   70
Dimensions:   Width: 15.60cm , Height: 2.80cm , Length: 23.40cm
Weight:   0.858kg
ISBN:  

9789027706997

ISBN 10:   9027706999
Pages:   465
Publication Date:   30 November 1976
Audience:   General/trade ,  Professional and scholarly ,  General ,  Professional & Vocational
Format:   Hardback
Publisher's Status:   Active
Availability:   Temporarily unavailable  
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Table of Contents

Introductory 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.

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