A comprehensive near- and far-ultraviolet spectroscopic study of the hot DA white dwarf G191-B2B
Constraining the magnetic field on white dwarf surfaces; Zeeman effects and fine structure constant variation
Hot DA white dwarf model atmosphere calculations: including improved Ni PI cross-sections
Limits on the Dependence of the Fine-Structure Constant on Gravitational Potential from White-Dwarf Spectra
Measuring chemical evolution and gravitational dependence of a using ultraviolet Fe v and Ni v transitions in white-dwarf spectra
Measuring the fine-structure constant on a white dwarf surface; a detailed analysis of Fe V absorption in G191-B2B
Stark broadening effect in hot DA white dwarfs: Ultraviolet lines of Fe V
Stellar laboratories. III. New Ba v, Ba vi, and Ba vii oscillator strengths and the barium abundance in the hot white dwarfs G191-B2B and RE 0503-289
Stellar laboratories. II. New Zn iv and Zn v oscillator strengths and their validation in the hot white dwarfs G191-B2B and RE 0503-289
Stellar laboratories . VIII. New Zr iv-vii, Xe iv-v, and Xe vii oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191-B2B and RE 0503-289
Stellar laboratories. VI. New Mo iv-vii oscillator strengths and the molybdenum abundance in the hot white dwarfs G191-B2B and RE 0503-289
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
The Structure of the Local Interstellar Medium. V. Electron Densities
The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. I. NLTE spectral analysis of the DA-type white dwarf G191-B2B
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2001-09-12T20:59:31Z/2001-09-19T22:20:36Z
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.
