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Deuterium abundance and background radiation temperature in high-redshift primordial clouds
scientific article published in Nature
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title
Deuterium abundance and background radiation temperature in high-redshift primordial clouds
(English)
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author name string
A. Songaila
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1
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L. L. Cowie
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2
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C. J Hogan
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3
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M. Rugers
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4
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language of work or name
English
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publication date
April 1994
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published in
Nature
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volume
368
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issue
6472
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page(s)
599–603
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exact match
https://scigraph.springernature.com/pub.10.1038/368599a0
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cites work
A preliminary measurement of the cosmic microwave background spectrum by the Cosmic Background Explorer (COBE) satellite
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https://api.crossref.org/works/10.1038%2F368599A0
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7 January 2021
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Measurement of the cosmic microwave background spectrum by the COBE FIRAS instrument
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Structure in the COBE differential microwave radiometer first-year maps
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Primordial Helium Abundance and the Primordial Fireball. II
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The origin of deuterium
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Primordial nucleosynthesis redux
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Galactic evolution of D and He-3
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The primordial helium abundance from observations of extragalactic HII regions
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THE PROGENITORS OF GALAXIES AND THE GAS CONTENT OF THE UNIVERSE AT LARGE REDSHIFTS.
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On measuring the deuterium abundance in QSO obsorption systems
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The case for the relativistic hot Big Bang cosmology
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Interstellar cyanogen and the temperature of the cosmic microwave background radiation
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Fine-structure transitions
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An upper limit on the microwave background temperature at z = 1.776
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A survey of Lyman-limit absorption in the spectra of 59 high-redshift QSOs
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High-resolution spectroscopy of selected absorption lines toward quasi-stellar objects. II. The metal-hydrogen ratio in a "metal-free" cloud toward S5 0014+81
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On the abundance of metals and the ionization state in absorbing clouds toward QSOs
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New photoionization models of interacgalactic clouds
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Goddard high-resolution spectrograph observations of the local interstellar medium and the deuterium/hydrogen ratio along the line of sight toward Capella
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Measurements of the 3He abundance in the interstellar medium
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The baryon content of galaxy clusters: a challenge to cosmological orthodoxy
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Possible gravitational microlensing of a star in the Large Magellanic Cloud
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Identifiers
DOI
10.1038/368599A0
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ADS bibcode
1994Natur.368..599S
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Dimensions Publication ID
1028186989
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