TY - BOOK ID - 100267996 TI - Asymmetric Planetary Nebulae VII AU - Parker, Quentin A. AU - Soker, Noam PY - 2019 SN - 3038976415 3038976407 PB - MDPI - Multidisciplinary Digital Publishing Institute DB - UniCat KW - UIE bands KW - stars: binaries KW - X-rays KW - binary stars KW - planetary systems KW - abundances KW - post-AGB KW - normal modes KW - theory and observation KW - binaries: spectroscopic KW - stellar evolution KW - binaries: close KW - AGB stars KW - stars: individual: WD 1751+106 KW - displacement vectors KW - AGB and post-AGB KW - extinction KW - circumstellar matter KW - stars: individual: WD 2134+25 KW - asymptotic giant branch stars KW - winds and outflows KW - ISM: abundances KW - stars: AGB and post-AGB KW - late stage stellar evolution KW - central stars of planetary nebulae KW - ultraviolet radiation KW - supernovae KW - stellar mass loss KW - circumstellar dust KW - integral field spectroscopy KW - planetary nebulae KW - radial velocity KW - mass-loss KW - pre-PN hydrodynamic models KW - infra-red KW - planetary nebulae: Common Envelope KW - astrochemistry KW - dust KW - multi-wavelength photometry KW - ISM: jets and outflows KW - planetary nebulae: individual (OH231+8+04.2) KW - radio continuum KW - stars: abundances KW - shock wave KW - stars: individual: WD 0044–121 KW - post-AGB stars KW - proto-planetary nebulae KW - binarity: transients: planetary nebulae KW - stars: atmospheres KW - stars: variables: general KW - AGB and post-AGB stars KW - jets KW - (sub)millimeter interferometry KW - discs KW - binarity KW - winds KW - observations KW - mass loss KW - X-ray KW - stars: winds KW - aperture masking KW - outflows KW - fullerenes KW - planetary nebula KW - pulsation KW - interstellar medium KW - planetary nebulae: individual (NGC 6781) KW - late-stage stellar evolution KW - infrared interferometry KW - accretion disks UR - https://www.unicat.be/uniCat?func=search&query=sysid:100267996 AB - 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. ER -