NGC 1992: Difference between revisions
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Silverleaf81 (talk | contribs) Rescuing 1 sources and tagging 0 as dead.) #IABot (v2.0.9.5 |
make apparent size specification consistent, add unit, fix parameter name for apparent size |
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| appmag_b = 14.65 <ref name="NGC 1992 - Apparent magnitude">{{cite web|url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+1992&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|title=NGC 1992|work=NED|access-date=22 November 2017}}</ref> |
| appmag_b = 14.65 <ref name="NGC 1992 - Apparent magnitude">{{cite web|url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+1992&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|title=NGC 1992|work=NED|access-date=22 November 2017}}</ref> |
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| appmag_v = 13.8<ref name="Apparent mag">{{cite web|url=http://spider.seds.org/ngc/revngcic.cgi?NGC1992|title=Object: NGC 1992 (*)|work=SEDS|access-date=22 November 2017}}</ref> |
| appmag_v = 13.8<ref name="Apparent mag">{{cite web|url=http://spider.seds.org/ngc/revngcic.cgi?NGC1992|title=Object: NGC 1992 (*)|work=SEDS|access-date=22 November 2017}}</ref> |
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| size_v = |
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| h_radial_v = 10601 +/- 45<ref name="NGC 1992 - Apparent magnitude"/> |
| h_radial_v = 10601 +/- 45<ref name="NGC 1992 - Apparent magnitude"/> |
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| constellation name = [[Columba (constellation)|Columba]] |
| constellation name = [[Columba (constellation)|Columba]] |
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| dist_ly= 473 million |
| dist_ly= 473 million |
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| dist_pc = |
| dist_pc = |
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| names = ESO 423- G 023, AM 0532-305, 2MASX J05343177-3053492, PGC 017466 <ref name="NGC 1992 - Apparent magnitude"/> |
| names = ESO 423- G 023, AM 0532-305, 2MASX J05343177-3053492, PGC 017466 <ref name="NGC 1992 - Apparent magnitude"/>}} |
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|image_size=250}} |
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'''NGC 1992''' (also known as '''PGC 17466''') is a [[lenticular galaxy]] located in the [[Columba (constellation)|Columba]] constellation. It was discovered by [[John Herschel]] on November 19, 1835.<ref>{{cite web|url=http://cseligman.com/text/atlas/ngc19a.htm#1992|title=NGC 1992|work=cseligman|access-date=22 November 2017}}</ref> It is about 473 million light years from the [[Milky Way]], Its apparent magnitude is 14.65 and its size is 1. |
'''NGC 1992''' (also known as '''PGC 17466''') is a [[lenticular galaxy]] located in the [[Columba (constellation)|Columba]] constellation. It was discovered by [[John Herschel]] on November 19, 1835.<ref>{{cite web|url=http://cseligman.com/text/atlas/ngc19a.htm#1992|title=NGC 1992|work=cseligman|access-date=22 November 2017}}</ref> It is about 473 million light years from the [[Milky Way]], Its apparent magnitude is 14.65 and its size is 1.0 x 0.7 [[Minute and second of arc|arc minutes]].<ref name="NGC 1992 - Apparent magnitude"/> |
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==References== |
==References== |
Latest revision as of 16:33, 24 December 2024
NGC 1992 | |
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Observation data (J2000.0 epoch) | |
Constellation | Columba |
Right ascension | 05h 34m 31.8s[1] |
Declination | −30° 53′ 49″[1] |
Redshift | 0.035361 +/- 0.000150[2] |
Heliocentric radial velocity | 10601 +/- 45[2] |
Distance | 473 million |
Apparent magnitude (V) | 13.8[3] |
Apparent magnitude (B) | 14.65 [2] |
Characteristics | |
Type | SA0/a?(rs) |
Apparent size (V) | 1.0 x 0.7 arc minutes[2] |
Other designations | |
ESO 423- G 023, AM 0532-305, 2MASX J05343177-3053492, PGC 017466 [2] |
NGC 1992 (also known as PGC 17466) is a lenticular galaxy located in the Columba constellation. It was discovered by John Herschel on November 19, 1835.[4] It is about 473 million light years from the Milky Way, Its apparent magnitude is 14.65 and its size is 1.0 x 0.7 arc minutes.[2]
References
[edit]- ^ a b "Galaxy NGC 1992". DSO. Archived from the original on 1 December 2017. Retrieved 22 November 2017.
- ^ a b c d e f "NGC 1992". NED. Retrieved 22 November 2017.
- ^ "Object: NGC 1992 (*)". SEDS. Retrieved 22 November 2017.
- ^ "NGC 1992". cseligman. Retrieved 22 November 2017.