Low surface brightness galaxy
A low-surface-brightness galaxy, or LSB galaxy, is a diffuse galaxy with a surface brightness that, when viewed from Earth, is at least one magnitude lower than the ambient night sky.
Most LSBs are dwarf galaxies, and most of their baryonic matter is in the form of neutral gaseous hydrogen, rather than stars. They appear to have over 95% of their mass as non-baryonic dark matter. There appears to be little supernova (SN) activity in these galaxies,[citation needed] although LSB galaxy IC 217 hosted 2014cl.[2][3]
In comparison to the high-surface-brightness galaxies, LSBs are mainly isolated
LSB galaxies were theorized to exist in 1976 by Mike Disney.
Giant low-surface-brightness galaxies
Giant low surface brightness (GLSB) galaxies are among the most massive known
UGC 1382 was previously thought to be an elliptical galaxy, but low-brightness spiral arms were later detected. UGC 1382 is much closer to Earth than Malin 1.[7]
Examples
See also
References
- ^ "Hiding in the night sky". Retrieved 4 April 2016.
- .
- Bibcode:2014CBET.3950....1G.
- ^ S2CID 118546432.
- ^ Bibcode:1997SciAm.276b..40B
- ^ Ken Crosswell, "Malin 1: A Bizarre Galaxy Gets Slightly Less So", 22 January 2007
- ^ "Surprise: Small elliptical galaxy actually a giant disk". 11 July 2016. Retrieved 12 July 2016.
- K. O'Neil, The HI Content and Extent of Low Surface Brightness Galaxies - Could LSB Galaxies be Responsible for Damped Ly-alpha Absorption?. For publication in Extragalactic Gas at Low Redshift, by Mulchaey, et al., eds (2001).
- S.D. Rosenbaum and D.J. Bomans, The environment of Low Surface Brightness Galaxies. Astronomy & Astrophysics Letters, 422, 5-8 (2004).
- A.J. Barth, A normal stellar disk in the galaxy Malin 1. Astronomical Journal133, 1085-1091 (2007).