Lyons Groups of Galaxies
{{Short description|Astronomical catalogue}}
Lyons Groups of Galaxies (or LGG) is an astronomical catalog of nearby groups of galaxies complete to a limiting apparent magnitude B0=14.0 with a recession velocity smaller than 5,500 km/s. The catalogue was obtained from the Lyon-Meudon Extragalactic Database. Two methods were used in group construction: a percolation method derived from Huchra and Geller {{cite journal
| last1 = Huchra
| first1 = J. P.
| last2 = Geller
| first2 = M. J.
|date=June 1982
| title = Groups of galaxies. I - Nearby groups
| journal = Astrophysical Journal
| series = Part 1
| volume = 257
| issue = June 15, 1982
| pages = 423–437
| bibcode = 1982ApJ...257..423H
| doi = 10.1086/160000
| accessdate = March 24, 2012
| url = http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1982ApJ...257..423H&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf
}} and a hierarchical method initiated by R. Brent Tully.{{cite journal
| last1 = Tully
| first1 = R. B.
| authorlink1 = R. B. Tully
|date=April 1980
| title = Nearby groups of galaxies. I - The NGC 1023 group
| journal = Astrophysical Journal
| series = Part 1
| volume = 237
| issue = Apr. 15, 1980
| pages = 390–403
| bibcode = 1980ApJ...237..390T
| doi = 10.1086/157881
| accessdate = March 24, 2012
| url = http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1980ApJ...237..390T&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf
}} The catalog is a synthesized version of the two results.
The LGG includes 485 groups and 3,933 member galaxies.
See also
References
{{reflist}}
External links
- [http://cdsarc.u-strasbg.fr/viz-bin/Cat?J/A%2bAS/100/47 LGG description at CDS]
- [http://webviz.u-strasbg.fr/viz-bin/VizieR-4?-out.max=999&-source=J/A%2BAS/100/47/table1 Full LGG list of records at CDS]
- [http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?1993A%26AS..100...47G ADS: General study of group membership. II - Determination of nearby groups]
Category:Astronomical catalogues of galaxy clusters
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