Abundance studies of sdB stars using UV echelle HST/STIS spectroscopy
A Low-metallicity Molecular Cloud in the Lower Galactic Halo
Beyond the iron group: Heavy metals in hot subdwarfs
Detection of a companion to the pulsating sdB Feige 48
HST/STIS observations of sdBV stars: testing diffusion and pulsation theory
Improved Determination of the Atmospheric Parameters of the Pulsating sdB Star Feige 48
The Chemical Composition of Subdwarf B Stars: Spectroscopic Diagnostics and Clues to Evolution
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2001-03-26T05:01:09Z/2002-02-17T19:28:15Z
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, Heber comma Ulrich, 2006, 'A test of pulsation and diffusion theory for subluminous B stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-mv25ohs