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The distribution of Lyman-alpha absorption lines in the spectra of six QSOs - Evidence for an intergalactic origin
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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Citations
Cited by
Tumlinson, J., Peeples, M. S., & Werk, J. K. (2017) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-091916-055240 · Cited by 1,147
The Lyman-Alpha Forest in the Cold Dark Matter Model
Hernquist, Katz, Weinberg, & Miralda-Escudé, J. (1996) · The Astrophysical Journal · doi:10.1086/309899 · Cited by 438
Metadata
- Authors
- Sargent, W. L. W., Young, P. J., Boksenberg, A., & Tytler, D.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- 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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- 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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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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