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The distribution of Lyman-alpha absorption lines in the spectra of six QSOs - Evidence for an intergalactic origin

Sargent, W. L. W., Young, P. J., Boksenberg, A., Tytler, D.·1980·The Astrophysical Journal Supplement Series

Abstract

The large Lyman-alpha samples in five QSOs with zem between 2.2 and 3.3 are used to test whether the absorbing gas is cosmologically distributed or ejected from the QSOs. It is shown that there is no significant variation in line density with redshift, nor in the rest equivalent width spectrum among the QSOs. In addition, the mean number density of lines in each object is found to be the same, that is, 60 lines per delta z=1 with W greater than or equal to 0.32 A.

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Metadata

Authors
Sargent, W. L. W., Young, P. J., Boksenberg, A., & Tytler, D.
Venue
The Astrophysical Journal Supplement Series
Published
1980-01
Volume
42
Pages
41
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W1999911662
Cited by
331
References
0
Type
conference abstract
Language
en
Open access
closed

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CoChat. (2026). Citation check: The distribution of Lyman-alpha absorption lines in the spectra of six QSOs - Evidence for an intergalactic origin. https://app.cochat.ai/papers/10.1086/190644
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Sargent, W. L. W., Young, P. J., Boksenberg, A., & Tytler, D. (1980). The distribution of Lyman-alpha absorption lines in the spectra of six QSOs - Evidence for an intergalactic origin. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/190644

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