An Atlas of N II and O III Images and Spectra of Planetary Nebulae
Determination of Planetary Nebulae angular diameters from radio continuum spectral energy distribution modelling
Expansion patterns and parallaxes for planetary nebulae
Filaments as Possible Signatures of Magnetic Field Structure in Planetary Nebulae
Hubble Space Telescope Expansion Parallaxes of the Planetary Nebulae NGC 6578, NGC 6884, NGC 6891, and IC 2448
Low-ionization structures in planetary nebulae - I. Physical, kinematic and excitation properties
Morphokinematic modelling of the point-symmetric Cats Eye, NGC 6543: Ring-like remnants of a precessing jet
NGC 6543. II. Understanding the Dilation of the Cats Eye
Physical Structure of Planetary Nebulae. II. NGC 7662
Proper Motion and Kinematics of the Ansae in NGC 7009
Rings and arcs around evolved stars - II. The Carbon Star AFGL 3068 and the Planetary Nebulae NGC 6543, NGC 7009, and NGC 7027
The 3-D ionization structure and evolution of NGC 7009 (Saturn Nebula)
The 3D velocity structure of the planetary nebula NGC 7009
Unveiling shocks in planetary nebulae
Young Planetary Nebulae: Hubble Space Telescope Imaging and a New Morphological Classification System
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-10-07T18:47:13Z/2001-05-11T19:46:14Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Hajian comma Arsen R., 2002, 'Expansion Parallax Distances to Planetary Nebulae', 1.0, European Space Agency, https://doi.org/10.5270/esa-36rr13u