damped Lyman-alpha systems

E451580

Damped Lyman-alpha systems are high-column-density neutral hydrogen gas clouds observed in quasar spectra, serving as key probes of the interstellar medium and chemical evolution of galaxies in the early universe.

All labels observed (1)

Label Occurrences
damped Lyman-alpha systems canonical 1

How this entity was disambiguated

Statements (48)

Predicate Object
instanceOf astrophysical object ⓘ
neutral hydrogen absorber ⓘ
quasar absorption line system ⓘ
causes depletion of refractory elements onto dust grains ⓘ
constrains cosmic evolution of neutral hydrogen density ⓘ
nucleosynthesis yields of early generations of stars ⓘ
contains dust ⓘ
contrastedWith Lyman-alpha forest absorbers ⓘ
Lyman-limit systems ⓘ
definedBy high-column-density neutral hydrogen gas ⓘ
hasAbbreviation DLA ⓘ
hasAlternativeName damped Lyα system ⓘ
hasCosmologicalSignificance dominant reservoir of neutral gas at high redshift ⓘ
hasEnvironment often associated with faint or low-luminosity galaxies ⓘ
hasKinematics multiple narrow velocity components ⓘ
velocity widths of tens to hundreds of km s^-1 ⓘ
hasLowerColumnDensityLimitThan sub-damped Lyman-alpha systems ⓘ
hasLymanAlphaProfile damped wings ⓘ
hasMetallicity sub-solar metallicity ⓘ
typically 1/100 to 1/3 solar ⓘ
hasNeutralHydrogenColumnDensity > 10^20.3 atoms cm^-2 ⓘ
> 2×10^20 atoms cm^-2 ⓘ
hasObservationTechnique high-resolution optical and UV spectroscopy ⓘ
hasOpticalDepth optically thick at the Lyman limit ⓘ
hasPhysicalComponent neutral hydrogen gas cloud ⓘ
hasRedshiftRange z ~ 0–5 and above ⓘ
hasSelectionMethod absorption-selected in background source spectra ⓘ
hasTypicalRedshiftRange high redshift (z ≳ 2) ⓘ
locatedIn circumgalactic medium ⓘ
interstellar medium of galaxies ⓘ
measuredBy Voigt profile fitting of Lyman-alpha line ⓘ
curve-of-growth analysis of metal lines ⓘ
observedIn gamma-ray burst afterglow spectrum ⓘ
quasar spectrum ⓘ
probes chemical evolution of galaxies ⓘ
cosmic neutral gas content ⓘ
interstellar medium in high-redshift galaxies ⓘ
star-formation fuel in the early universe ⓘ
relatedTo sub-damped Lyman-alpha system ⓘ
showsSpectralFeature Lyman series absorption lines ⓘ
damped Lyman-alpha absorption line ⓘ
metal absorption lines ⓘ
traces neutral gas reservoir for star formation ⓘ
usedAs probe of galaxy formation ⓘ
probe of large-scale structure ⓘ
tracer of cosmic metal enrichment ⓘ
usedToMeasure abundances of elements such as Fe, Si, Zn, S ⓘ
primordial deuterium abundance in some cases ⓘ

How these facts were elicited

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

MIKE → scienceTarget → damped Lyman-alpha systems ⓘ