Spectroscopic Survey of Faint Planetary-nebula Nuclei. V. The EGB 6-type Central Star of Abell 57
The hot white dwarf in the peculiar binary nucleus of the planetary nebula EGB 6
The Nucleus of the Planetary Nebula EGB 6 as a Post-Mira Binary
Instrument
COS, COS/FUV, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2014-04-01T20:49:46Z/2014-04-01T22:38:15Z
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, Bond, 2015, 'Tol 26 and the EGB 6 Class of Planetary-Nebula Nuclei: What Happens to a Companion Star when a PN is Ejected?', 1.0, European Space Agency, https://doi.org/10.5270/esa-dynxgb5