A gigantic cloud of → hydrogen
hydrogen gas emitting the → Lyman alpha line
identified in → high redshift, → narrow band → surveys. LABs can span hundreds of thousands of
→ light-years that is larger than galaxies.
Normally, Lyman alpha emission is in the ultraviolet part of the spectrum, but Lyman alpha
blobs are so distant, their light is redshifted to (longer) optical wavelengths.
The most important questions in LAB studies remain unanswered: how are they formed and
what maintains their power?
One of the largest LABs known is SSA22-LAB-01 (z = 3.1).
Embedded in the core of a huge → cluster of galaxies
in the early stages of formation, it
was the very first such object to be discovered (in 2000) and is located so far away that
its light has taken about 11.5 billion years to reach us. Recent observations of
SSA22-LAB-01 using → ALMA
shows two galaxies at the core of this object and they are
undergoing a burst of → star formation
that is lighting up their surroundings.
These large galaxies are in turn at the centre of a swarm of smaller ones in what appears
to be an early phase in the formation of a massive cluster of galaxies
(see J. E. Geach et al. 2016, arXiv:1608.02941).
See also: → Lyman; → alpha;
→ blob.