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Lyman-break galaxy

(LBG)
(a galaxy emitting very little shorter than 912 angstroms)

A Lyman-break galaxy (LBG) is a galaxy identified as star forming by a Lyman break, a lack of radiation emitted with wavelength shorter than 912 angstroms, the Lyman limit, i.e., the lower limit on wavelengths in the Lyman series. Neutral hydrogen around star-forming regions absorbs the radiation.

This method of identifying star-forming galaxies is largely used at redshifts of z in the 3-to-4 range, using filters on the redshifted spectrum. The method has the advantage that the "break" causes dropouts, i.e., images through some filters don't show the galaxy, providing a relatively easy way to identify them by comparing the filtered images, that the break is visible through the Earth's atmosphere within the 3-4 redshift range, and that the redshift can be determined with some precision using subsequent spectrography to identify the wavelength of the observed break.


Note that the abbreviation LBG is also used for locally brightest galaxy.


(galaxy type)
Further reading:
https://en.wikipedia.org/wiki/Lyman-break_galaxy
http://burro.astr.cwru.edu/Academics/Astr328/Notes/GalForm/LyBreakTech.html
https://www.oxfordreference.com/display/10.1093/oi/authority.20110803100120968
http://ned.ipac.caltech.edu/level5/Giavalisco/Giav_contents.html
https://ned.ipac.caltech.edu/level5/Sept14/Dunlop/Dunlop3.html
PrefixExample  
LBGLBG J213512.73-010143general prefix for LBGs

Referenced by pages:
Balmer-break galaxy (BBG)
brightest cluster galaxy (BCG)
HD1
Lyman break (LB)
Lyman continuum (LyC)

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