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Angular Momentum and Mass Loss for Hot Stars

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Table of Contents

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    Book Overview
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    Chapter 1 Why a Meeting on Angular Momentum and Mass Loss for Hot Stars?
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    Chapter 2 The Effects of Rotation on Stellar Structure and Evolution
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    Chapter 3 New Evolutionary Aspects of Mass Loss and Angular Momentum
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    Chapter 4 Mass Loss during the Evolution of Massive Stars
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    Chapter 5 Angular Momentum Loss in Pre-Main Sequence Objects and the Initial Angular Momentum of Stars
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    Chapter 6 The Herbig Ae and Be Stars: Mass and Angular Momentum Losses
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    Chapter 7 Eccentric Spiral Modes in Disks Associated with Young Stellar Objects
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    Chapter 8 Evidence That Wolf-Rayet Stars are Pre-Main Sequence Objects
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    Chapter 9 Rotation, Pulsation and Atmospheric Phenomena in A—Type Stars
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    Chapter 10 Pulsation Studies of a 1.8 M ⊙ Delta Scuti Model
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    Chapter 11 Post-Main Sequence Evolution of Binary Am Stars
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    Chapter 12 A Statistical Study of Main Sequence A and F Stars: Testing the Main Sequence Mass Loss Hypothesis
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    Chapter 13 Basic Magnetic Rotator Theory with Application to the Angular Momentum Driven Winds of B[e] and Wolf Rayet Stars
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    Chapter 14 The Connection between Rotation and the Winds of Be Stars
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    Chapter 15 UV Glimpse of OB Stars
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    Chapter 16 Nonspherical Radiation Driven Wind Models Applied to Be Stars
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    Chapter 17 A Simple Criterion to Identify Rapidly Rotating Stars Viewed at Small to Intermediate Inclination Angles
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    Chapter 18 Intensive Photometric Campaign on Be Stars: Behaviour of Short-Term Periodic Variations and Its Relationship to Pulsation and Mass Loss
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    Chapter 19 Constraints on the Thickness of be Star Disks Derived from Combined IR Excess and Optical Polarimetry Data
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    Chapter 20 On the Correlation between Pulsation Amplitude and Shell Activity in the Be Star λ Eridani
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    Chapter 21 B[e] Supergiants: Continuum Polarization by Electron Scattering in Rotationally Distorted, Radiation Driven Stellar Winds
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    Chapter 22 Rotational Evolution of Hot Stars Due to Mass Loss and Magnetic Fields
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    Chapter 23 New Facts about the Variability of 45 ɛ Persei
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    Chapter 24 Long-term study of stellar-wind variability of O stars
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    Chapter 25 He II λ1640 as a Diagnostic for Assessing the Extent of Rapid Rotation in Be Stars
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    Chapter 26 Some Examples of the Role of Stellar Rotation in Hot Star Winds
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    Chapter 27 HD193077—A Fast Rotating Wolf-Rayet Star
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    Chapter 28 How Effective is Rotation in Enhancing the Rate of Mass Loss in Early Type Stars?
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    Chapter 29 Rotation and Pulsation—Mode—Selection in B—Type Stars
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    Chapter 30 The Angular Momentum-Loss and the Differential Rotation in B and Be Stars
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    Chapter 31 The Role of Axial Symmetry in the Upper Part of the HRD: B[e] Supergiants and LBVs
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    Chapter 32 Effects of Mass Loss on Late Stages of Massive Star Evolution
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    Chapter 33 V444 Cygni and CQ Cephei, Key Wolf-Rayet Binary Stars
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    Chapter 34 Rotation of Hot Stars after They Cool Off
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    Chapter 35 Winds, Mass Loss and Rotation in Central Stars of Planetary Nebulae
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    Chapter 36 White Dwarf Mass Loss, Rotation, Individual Masses and the Identification of the White Dwarf Remnants of Upper Main Sequence Stars
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    Chapter 37 Evolved Stars as Probes of Main Sequence Angular Momentum and Mass Loss
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    Chapter 38 The Bizarre Kinematics of Planetary Nebula NGC 7009, and Some Thoughts on the Transfer of Stellar Angular Momentum to Planetary Nebulae
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    Chapter 39 Chromospheric H α Activity in α ORI
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    Chapter 40 Stellar Winds in A-Type Supergiants
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    Chapter 41 The Evidence That Wolf-Rayet Stars are in a Late Stage of Evolution
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    Chapter 42 Why Wolf-Rayet Stars should not be Considered to be Evolved Cores of Massive Stars
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Title
Angular Momentum and Mass Loss for Hot Stars
Published by
Springer Netherlands, December 2012
DOI 10.1007/978-94-009-2105-4
ISBNs
978-9-40-107446-9, 978-9-40-092105-4
Editors

Willson, L. A., Stalio, R.

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 1 Mendeley reader of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 1 100%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 1 100%
Readers by discipline Count As %
Physics and Astronomy 1 100%