Absolute spectrophotometry of northern compact planetary nebulae
Asymmetry of planetary nebulae: Collimated ionized jets in butterfly nebulae and dust extinction effects in compact planetary nebulae
A systematic study of young multipolar planetary nebulae
Determination of Planetary Nebulae angular diameters from radio continuum spectral energy distribution modelling
Discovery of Multiple Coaxial Rings in the Quadrupolar Planetary Nebula NGC 6881
Dust Extinction in Compact Planetary Nebulae
Hubble Space Telescope Observations and Geometric Models of Compact Multipolar Planetary Nebulae
Multipolar planetary nebulae: Not as geometrically diversified as thought
Multipolar Planetary Nebulae: Not as Geometrically Diversified as Thought
Rings and arcs around evolved stars - I. Fingerprints of the last gasps in the formation process of planetary nebulae
Rings in the haloes of planetary nebulae
Unveiling shocks in planetary nebulae
Young Planetary Nebulae: Hubble Space Telescope Imaging and a New Morphological Classification System
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-10-31T10:45:13Z/2000-02-20T01:40:34Z
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, Kwok comma Sun, 2001, 'Morphology of High Radio Surface Brightness Planetary Nebulae', 1.0, European Space Agency, https://doi.org/10.5270/esa-2fgykyx