Evidence for Deuterium Astration in the Planetary Nebula Sh 2-216?
Far-Ultraviolet Spectroscopic Analyses of Four Central Stars of Planetary Nebulae
High-resolution FUSE and HST ultraviolet spectroscopy of the white dwarf central star of Sh 2-216
Metal Absorption Profiles from the Central Star of the Planetary Nebula M27 (NGC 6853, PN G060.8-03.6, the Dumbbell): Photospheric and Nebular Line Identifications
Molecular and Atomic Excitation Stratification in the Outflow of the Planetary Nebula M27
The winds of hydrogen-rich central stars of planetary nebulae
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-10-24T17:55:53Z/2002-01-07T14:34:03Z
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, Werner comma Klaus, 2007, 'Temperature scale and metal abundances of hot hydrogen-rich central stars of planetary nebulae', 1.0, European Space Agency, https://doi.org/10.5270/esa-6uhqza3