A Detailed look at Chemical Abundances in Magellanic Cloud Planetary Nebulae. I. The Small Magellanic Cloud
A new population of planetary nebulae discovered in the Large Magellanic Cloud - III. The luminosity function
A new population of planetary nebulae discovered in the Large Magellanic Cloud - I. Preliminary sample
A new population of planetary nebulae discovered in the Large Magellanic Cloud (IV): the outer LMC
Euclid preparation. XXVII. A UV-NIR spectral atlas of compact planetary nebulae for wavelength calibration
Hubble Space Telescope Images of Magellanic Cloud Planetary Nebulae
Hubble Space Telescope Observations of Three Very Young Star Clusters in the Small Magellanic Cloud
Space Telescope Imaging Spectrograph Slitless Observations of Small Magellanic Cloud Planetary Nebulae: A Study on Morphology, Emission-Line Intensity, and Evolution
The Low- and Intermediate-Mass Stellar Population in the Small Magellanic Cloud: The Central Stars of Planetary Nebulae
Instrument
STIS/CCD
Temporal Coverage
2000-08-08T10:56:29Z/2001-05-16T01:14:24Z
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, Stanghellini comma Letizia, 2001, 'Survey of SMC Planetary Nebulae: Nebular and Stellar Evolution in a Low- Metallicity Environment', 1.0, European Space Agency, https://doi.org/10.5270/esa-r9j5dgl