Chapter
4 Time-dependent AGB winds
5 AGB evolution and binary mass transfer
The physical theory of winds from hot stars
3 The Wolf-Rayet wind momentum problem — a solution
4 Successes and failures of modified CAK theory
5 Wind-shocking and time-dependent theory
Axisymmetric Outflows from Single and Binary Stars
2 The Shaping of Planetary Nebulae
3 Mechanisms that Can Produce a Density Contrast or Axially Symmetric Outflows
3.1 Common Envelope Evolution
3.3 Rotation and Be Stars
3.4 Rotation and AGB Stars—Common Envelopes,Planets and Brown Dwarfs
3.4-1 Spin-up in a CE phase
3.4-2 Spin-up by brown dicarfs and planets
4 Accretion Disks in Post Common Envelope Binaries
Flows in Clumpy Circumstellar Media
2 Effects on Large Scale Flows
4 Planetary Nebula Dynamics
5 Intermediate Length-Scale Structures-Tails
6 Tails in the PNe NGC 7293
7 The Tail of the M Supergiant IRS7
8 Boundary Layer Diagnostics
Part two: Wolf-Rayet Ring Nebulae
Ring Nebulae around LBVs and WR stars
3 Formation of LBV and WR nebulae
5 The connection between LBV and WR nebulae
The Interstellar Environment of Wolf-Rayet Stars in the LMC: New Survey and Statistics
Morphology & Physical Conditions in WR Shell Nebulae
Three-Wind Model for Wolf-Rayet Bubbles
2 Technique and simulation
High Resolution Coronographic Imaging and Echelle Observations of S119: a new Luminous Blue Variable?1
2 High Resolution Echelle Observations
2.1 The Systemic Velocity
4 Is S119 a new Luminous Blue Variable?
New HST images of Eta Carinae and its surrounding nebulosity
2 Observations and Data Processing
3 Morphology of the Homunculus
Observations of Circumstellar Media Around Supernovae
3.2 SN 1988Z in MCG 03-28-022
Radio Supernovae as Probes of Progenitor Winds
2 Modelling the Radio Emission
3 Mass-Loss Rates from the Progenitor Star Systems
4 Classes of Radio Supernovae
5 Variations on a Central Theme
Circumstellar Interaction in Supernovae
2 Observational evidence for circumstellar interaction
4 Early circumstellar interaction
5 Very late emission from supernovae
2D Hydrodynamic Models of Supernova Progenitor Winds
2 Interacting Winds Model
Supernovae with dense circumstellar winds
Compact Supernova Remnants
2 cSNRs, or SNRs evolving in a high density medium
3 Numerical hydrodynamic models
5 Comparison with observations
5.3 SN~1955 in M82 (41.9+58)
6 Conclusions and future prospects
The evolution of compact supernova remnants
2 Numerical Calculations and Results
2.2 Boundary and Initial Conditions
2.3 The Time Evolution of Compact SNRs
2.4 Comparison with Observations
4 Rapid X-Ray Variability in Compact SNRs
4-1 Analytical Description of the X-Ray Bursts.
Massive Supernovae in Binary Systems
2 Evolution of Massive Supernova Progenitors in Binaries
3 Hydrodynamics of Massive Supernovae in Binaries
4 Application to Recent Supernovae
The Progenitor of SN 1993J and its Mass-Loss History
Narrow optical emission lines from supernova 1993J
3.2 Profiles of other lines
4 Origin of the Ho emission
UV Spectroscopy of SN 1993J and Detection of Highly-Ionized Gas Close to the Progenitor
Ryle Telescope observations of the radio emission from SN 1993J
2 Observations and Results
The Early Radio Emission from SN 1993J
The circumstellar gas around SN 1987A and SN 1993J
X-ray emission from the collision of supernova ejecta with circumstellar matter:SN 1987A & SN 1993J
Observations of Interstellar and Intergalactic gas towards SN 1993J in M81
3 Identification of absorbing regions
3.1 Interstellar gas in M81
3.2 Interstellar gas in the Galaxy
3.3 High Positive velocity gas
Part four: Asymptotic Giant Branch stars
Mass Loss from Late Type Stars
2 Mass Loss from Late Type Stars
3 Levitating the stellar atmosphere
3.1 Shock waves in AGB Stars
3.2 Acoustic heating in red giants and supergiants
5 Dusty Winds Driven by Radiation Pressure
Kinematics and structure of the molecular envelopes around stars on the AGB and beyond
2 The physical characteristics of a "standard" CSE
3 Kinematics of the molecular gas
4 The density structure of the molecular gas
5 A possible scenario for the evolution of a CSE
Circumstellar Shells of Long-Period Variables:Dust Formation and Optical Appearance
2.1 Dynamical model calculations
2.2 Radiative transfer calculations
Observation of circumstellar shells with the IRAM telescopes
2 Molecular emission in IRC+10216
4 The very fast outflow in CRL 618
Part five: Planetary Nebulae
Morphology and kinematics of Planetary Nebulae
2.2 PNe in the Magellanic Clouds and globular clusters
2.3 IR, (sub)-mm, and radio
4 Symbiotics with nebulae
FLIERs in elliptical Planetary Nebulae
3 Physical properties of microstructures
4 Chemical properties of the microstructures
6 Discussion and Conclusions
Circumstellar Dust in Planetary Nebulae and Proto-Planetary Nebulae
2 Infrared spectra of young PN
3 Infrared spectra of PPN
4 When do the PAH molecules form?
HST Observations of Hydrogen-Poor Ejecta in Abell 30 and Abell 78:Evidence for Mass-Loaded Flows
2 HST Images of A30 and A78: Cometary Structures
3 HST Spectra of the Central Star of A78
The evolution of the neutral envelopes of planetary nebulae
2 The Molecular Gas in PNe
3 Clumps and the Atomic-Molecular Transition
Magnetic Shaping of Planetary Nebulae
The hydrodynamics of aspherical two-wind configurations
6 Use and abuse of models
Part six: Novae and Symbiotic Stars
Novae and related stars as tracers of mass loss
4-1 GK Persei - a nova super-remnant
Circumstellar scattering processes in symbiotic systems
1 Circumstellar matter in symbiotic stars
2 Scattering processes in the circumstellar environment of symbiotic stars
3 Polarisation in the Raman scattered lines
Stellar Evolution and Wind Theory
Wolf-Rayet stars and Luminous Blue Variables
Asymptotic Giant Branch Stars and their Envelopes
Novae and Symbiotic Stars