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Stars --- Mass loss (Astrophysics). --- Masses --- Congresses.

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This long-awaited graduate textbook, written by two pioneers of the field, is the first to provide a comprehensive introduction to the observations, theories and consequences of stellar winds. The rates of mass loss and the wind velocities are explained from basic physical principles. This book also includes chapters clearly explaining the formation and evolution of interstellar bubbles, and the effects of mass loss on the evolution of high- and low-mass stars. Each topic is introduced simply to explain the basic processes and then developed to provide a solid foundation for understanding current research. This authoritative textbook is designed for advanced undergraduate and graduate students and researchers seeking an understanding of stellar winds and, more generally, supersonic flows from astrophysical objects. It is based on courses taught in Europe and the US over the past twenty years and includes seventy problems (with answers) for coursework or self-study.

Stars --- Stellar winds. --- Mass loss (Astrophysics) --- Vents stellaires --- Perte de masse (Astrophysique) --- Mass loss (Astrophysics). --- Stellar winds --- Loss, Mass (Astrophysics) --- Astrophysics --- Masses --- Winds, Stellar --- Space plasmas --- Stellar activity --- Winds --- 524.5 --- 524.5 Interstellar medium. Galactic nebulae --- Interstellar medium. Galactic nebulae

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This book contains the best and most up-to-date contributions in the field of late stage stellar evolution, as presented at the APNVII conference in Hong Kong in December 2017. A total of 60 scientists from 20 countries gathered to present, listen, interact and discuss the most current issues and problems in planetary nebulae and related objects research. The emphasis of this influential series of meetings, which was the seventh occasion over the last 20 years, has always been on the hypothesized and observed physical shaping mechanisms of the ejected nebulae that have such wonderful and intriguing forms. This special Galaxies conference issue of fully refereed contributions brings together a representative compilation of the meeting presentations in paper form. It captures the current “snap shot” status of this research field in some real sense. Such proceedings are well received and can be used as a reference material by both participants and all others working in the field for years to come.

UIE bands --- stars: binaries --- X-rays --- binary stars --- planetary systems --- abundances --- post-AGB --- normal modes --- theory and observation --- binaries: spectroscopic --- stellar evolution --- binaries: close --- AGB stars --- stars: individual: WD 1751+106 --- displacement vectors --- AGB and post-AGB --- extinction --- circumstellar matter --- stars: individual: WD 2134+25 --- asymptotic giant branch stars --- winds and outflows --- ISM: abundances --- stars: AGB and post-AGB --- late stage stellar evolution --- central stars of planetary nebulae --- ultraviolet radiation --- supernovae --- stellar mass loss --- circumstellar dust --- integral field spectroscopy --- planetary nebulae --- radial velocity --- mass-loss --- pre-PN hydrodynamic models --- infra-red --- planetary nebulae: Common Envelope --- astrochemistry --- dust --- multi-wavelength photometry --- ISM: jets and outflows --- planetary nebulae: individual (OH231+8+04.2) --- radio continuum --- stars: abundances --- shock wave --- stars: individual: WD 0044–121 --- post-AGB stars --- proto-planetary nebulae --- binarity: transients: planetary nebulae --- stars: atmospheres --- stars: variables: general --- AGB and post-AGB stars --- jets --- (sub)millimeter interferometry --- discs --- binarity --- winds --- observations --- mass loss --- X-ray --- stars: winds --- aperture masking --- outflows --- fullerenes --- planetary nebula --- pulsation --- interstellar medium --- planetary nebulae: individual (NGC 6781) --- late-stage stellar evolution --- infrared interferometry --- accretion disks