FOS observations of G117-B15A and the blue edge of the ZZ Ceti instability strip.
Optical and Ultraviolet Analyses of ZZ Ceti Stars and Study of the Atmospheric Convective Efficiency in DA White Dwarfs
Temperature dependence of the Lyman a line wings in cool hydrogen-rich white dwarf atmospheres. Application to ZZ Ceti white dwarf spectra
Instrument
FOS/BL
Temporal Coverage
1992-11-11T19:43:19Z/1992-11-11T23:21:49Z
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, Koester comma Detlev G., 1993, 'THE BLUE EDGE OF THE ZZ CETI INSTABILITY STRIP', 1.0, European Space Agency, https://doi.org/10.5270/esa-sj2e4mp