Deuterium abundances
arXiv:astro-ph/9903043 · doi:10.1016/S1384-1076(99)00017-2
Abstract
We discuss the measurements of deuterium abundances in high redshift quasar absorbers, in the solar system and in the interstellar medium. We present new results that indicate spatial variations of the deuterium abundance in the interstellar medium at the level of 50% over scales possibly as small as 10 pc, and discuss plausible causes for the origin of these variations.
19 pages, 1 figure. To appear in New Astronomy, for the David N. Schramm memorial volume
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Cited by in corpus (26)
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- The cosmological baryon density from the deuterium to hydrogen ratio towards QSO absorption systems: D/H towards Q1243+3047
- Review of Big Bang Nucleosynthesis and Primordial Abundances
- Abundances of Deuterium, Oxygen, and Nitrogen in the Local Interstellar Medium: Overview of First Results from the Far Ultraviolet Spectroscopic Explorer Mission
- Two New Low Galactic D/H Measurements from FUSE
- The Deuterium-to-Hydrogen Ratio in a Low-Metallicity Cloud Falling onto the Milky Way
- The deuterium-to-oxygen ratio in the interstellar medium
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- Evolution of Deuterium, 3He and 4He in the Galaxy
- Deuterium astration in the local disc and beyond
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- FUSE determination of a low deuterium abundance along an extended sight line in the Galactic disk
- Deuterated hydrogen chemistry: Partition functions, Equilibrium constants and Transition intensities for the H3+ system
- Tiny-Scale Molecular Structures in the Magellanic Clouds (Part 1)
- FUSE Observations of the HD Molecule toward HD 73882
- Deuterium toward the WD0621-376 sight line: Results from the Far Ultraviolet Spectroscopic Explorer (FUSE) Mission
- Variations in the D/H ratio of extended sightlines from FUSE observations
- The D/H Ratio in the Interstellar Medium toward the White Dwarf PG0038+199
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- Deuterium at high redshift: primordial or evolved ?
- Stochastic processes, galactic star formation, and chemical evolution. Effects of accretion, stripping, and collisions in multiphase multi-zone models
- Cosmological History of Stars and Metals
- Modelling the chemical evolution of the Milky Way