Analysis of Co-spatial UV-optical HST/STIS Spectra of Planetary Nebula NGC 3242
Caught in the Act: Gas and Stellar Velocity Dispersions in a Fast Quenching Compact Star-Forming Galaxy at z~1.7
Co-spatial Long-slit UV/Optical AL Spectra of 10 Galactic Planetary Nebulae with HST/STIS. I. Description of the Observations, Global Emission-line Measurements, and CNO Abundances
Co-spatial Long-slit UV/Optical Spectra of Ten Galactic Planetary Nebulae with HST/STIS. II. Nebular Models, Central Star Properties, and He+CNO Synthesis
Co-spatial UV-optical HST/STIS spectra of six planetary nebulae: nebular and stellar properties
On the production of He, C, and N by low- and intermediate-mass stars: a comparison of observed and model-predicted planetary nebula abundances
UV spectral analysis of very hot H-deficient WCE-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2012-01-15T20:58:10Z/2013-01-28T06:21:26Z
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, Dufour comma Reginald J., 2014, 'Carbon and Nitrogen Enrichment Patterns in Planetary Nebulae', 1.0, European Space Agency, https://doi.org/10.57780/esa-jkhbkrf
