Lyman-alpha blob 1
Interstellar cloud
Intergalactic cloud
Polarized image of LAB-1, shown as the faint, green gas cloud.
Observation data: J2000 epoch
SubtypeLyman-alpha blob
Right ascension22h 17m 25.97s[1]
Declination+00° 12′ 38.9″[1]
Distance1.15 × 1010 ly
ConstellationAquarius
Physical characteristics
Radius150,000 ly
DesignationsSMM J221726+0013,[1] WBG2010 C11
See also: Lists of nebulae

Lyman-alpha blob 1 (LAB-1) is a giant cosmic cloud of gas located in the constellation of Aquarius, approximately 11.5 billion light-years from Earth with a redshift (z) of 3.09. It was discovered unexpectedly in 2000 by Charles Steidel and colleagues,[2] who were surveying for high-redshift galaxies using the 200 inch (5.08 m) Hale telescope at the Palomar Observatory.[3] The researchers had been investigating the abundance of galaxies in the young Universe when they came across two objects which would become known as Lyman-alpha blobs[2]—huge concentrations of gases emitting the Lyman-alpha emission line of hydrogen.[4]

LAB-1 is the first discovered Lyman-alpha blob, hence it has the number 1. It is the prototype of objects of this kind.[3] It is also one of the largest of its kind, measuring 300,000 light years across, three times larger than the Milky Way.[4] The blob appears green on the image because of the combination of the high redshift (z = 3) and the ultraviolet nature of the blob.[4] Imaging with the European Southern Observatory's Very Large Telescope showed that much of the light from the blob is polarized, the proportion increasing and peaking at around 20% at a radius of 45 kiloparsecs (145,000 light-years), forming a huge ring around the blob.[5]

It is still unclear as to why this object is emitting the Lyman-alpha emission radiation. It is thought that the light is coming from galaxies within the central region of the blob. Light of such intensities could be from active galaxies or supermassive black holes actively absorbing matter.[4] An alternate theory is that the light is from cooling gas falling into early galaxies, which has possibly come from cosmic filaments (as galaxies are thought to form at the intersections of these filaments), however the pattern of polarisation found argues against this.[2]

Gallery

Also See

SSA22 Protocluster


References

  1. ^ a b c "SMM J221726+0013". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^ a b c Bower, Richard (2011). "Unlocking the Secrets of the Giant Blobs". Nature. 476 (3760): 288–89. Bibcode:2011Natur.476..288B. doi:10.1038/476288a. ISSN 0028-0836. PMID 21850099.
  3. ^ a b Steidel, Charles C.; Adelberger, Kurt L.; Shapley, Alice E. (2000). "Lyα Imaging of a Proto–Cluster Region at z = 3.09". Astrophysical Journal. 532 (1): 170–82. arXiv:astro-ph/9910144. Bibcode:2000ApJ...532..170S. doi:10.1086/308568.
  4. ^ a b c d "Giant Space Blob Glows from Within". ESO Press Release. 17 August 2011. Retrieved 18 August 2011.
  5. ^ Hayes, Matthew; Scarlata, Claudia; Siana, Brian (2011). "Central powering of the largest Lyman-[alpha] nebula is revealed by polarized radiation". Nature. 476 (3760): 304–07. arXiv:1108.3332. Bibcode:2011Natur.476..304H. doi:10.1038/nature10320. ISSN 0028-0836. PMID 21850104. S2CID 4310494.
  6. ^ "ALMA Uncovers Secrets of Giant Space Blob". www.eso.org. Retrieved 23 September 2016.


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