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Simultaneously storing both spectral and spatial information, 3D spectroscopy offers a new way to tackle astrophysical problems, and opens up new lines of research. Since its inception in the eighties and early nineties, research in this field has grown enormously. Large telescopes all around the world are now equipped with integral field units, and two instruments of the James Webb Space Telescope will have integral field spectroscopic capabilities. Nowadays, more effort is dedicated to refining techniques for reducing, analysing and interpreting the data obtained with 3D spectrographs. Containing lectures from the seventeenth Winter School of the Canary Islands Astrophysics Institute, this book explores 3D spectroscopy techniques and data. A broad and balanced presentation of research in this field, it introduces astronomers to a new generation of instruments, widening the appeal of integral field spectroscopy and helping it become a powerful tool in tackling astrophysical problems.

Astronomical spectroscopy --- Integral field spectroscopy --- Three-dimensional imaging in astronomy --- Three-dimensional astronomical imaging --- Imaging systems in astronomy --- Spectrum analysis --- Spectroscopie astronomique.

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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