Absorption measurements of Galaxy halos
EAS Publications Series, ISSN: 1633-4760, Vol: 56, Page: 225-230
2012
- 1Citations
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Metrics Details
- Citations1
- Citation Indexes1
- CrossRef1
Conference Paper Description
The analysis of hydrogen and metal absorption lines in the spectra of distant quasars (QSOs) has become a powerful method to study the distribution and physical properties of low-density gas situated in the extended halos and circumgalactic environment of galaxies at low and high redshift. We here review the overall properties of halo absorption-line systems seen in QSO spectra and discuss their connection to the Milky Way's population of intermediate- and high-velocity clouds. © EAS, EDP Sciences 2012.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84883403754&origin=inward; http://dx.doi.org/10.1051/eas/1256036; http://www.eas-journal.org/10.1051/eas/1256036; http://www.eas-journal.org/10.1051/eas/1256036/pdf; https://dx.doi.org/10.1051/eas/1256036; https://www.eas-journal.org/articles/eas/abs/2012/04/eas1256036/eas1256036.html
EDP Sciences
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