Discovery of photospheric Ca X emission lines in the far-UV spectrum of the hottest known white dwarf (KPD 0005+5106)
High ions towards white dwarfs: circumstellar line shifts and stellar temperature
HST STIS Observations of the Mixing Layer in the Cats Eye Nebula
Independent Emission and Absorption Abundances for Planetary Nebulae
Non-Local Thermodynamic Equilibrium Model of NGC 6543s Central Star and Its Relation to the Surrounding Planetary Nebula
Quantitative Spectral Analysis of Evolved Low-Mass Stars
StarCAT: A Catalog of Space Telescope Imaging Spectrograph Ultraviolet Echelle Spectra of Stars
The dense and asymmetric central star wind of the young PN He 2-138
The winds of hydrogen-rich central stars of planetary nebulae
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2003-09-16T16:51:05Z/2004-08-02T23:52:29Z
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, Williams comma Robert E., 2007, 'Integrated Absorption- and Emission-Line Analysis of Nebulae', 1.0, European Space Agency, https://doi.org/10.5270/esa-y0clajy
