Mode Identification in Pulsating White Dwarfs Using the HST
Mode Identification of Pulsating White Dwarfs Using the Hubble Space Telescope
Observations of the Pulsating White Dwarf G 185-32
Star cluster formation and evolution in the dwarf starburst galaxy NGC 1569
Temperature dependence of the Lyman a line wings in cool hydrogen-rich white dwarf atmospheres. Application to ZZ Ceti white dwarf spectra
The ZZ Ceti star G 185-32: new insight from asteroseismology
Instrument
FOS/BL
Temporal Coverage
1995-07-31T08:42:51Z/1995-08-01T01:28:27Z
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, Clemens comma James Christopher, 1996, 'TIME-RESOLVED SPECTROSCOPY OF THE PULSATING DA WHITE DWARF PY VUL', 1.0, European Space Agency, https://doi.org/10.5270/esa-41cb1zf