Mode Identification in Pulsating White Dwarfs Using the HST
Mode Identification of Pulsating White Dwarfs Using the Hubble Space Telescope
Temperature dependence of the Lyman a line wings in cool hydrogen-rich white dwarf atmospheres. Application to ZZ Ceti white dwarf spectra
The Pulsating White Dwarf Stars
Instrument
FOS/BL
Temporal Coverage
1994-09-20T01:28:45Z/1995-12-13T01:50:17Z
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, Nather comma R. Edward, 1996, 'TIME-RESOLVED SPECTROSCOPY OF THE PULSATING DA WHITE DWARF DN DRACONIS: CYCLE4 MEDIUM', 1.0, European Space Agency, https://doi.org/10.5270/esa-gt2kcr9