Editing IC 342/Maffei Group (section)

==Members==

The table below lists galaxies that have been identified as associated with the IC342/Maffei 1 Group by I. D. Karachentsev.<ref name="karachentsev2005" /><ref name=Karachentsev2020>{{cite journal|doi=10.1051/0004-6361/202037993|title=KKH 22, the first dwarf spheroidal satellite of IC 342|year=2020|last1=Karachentsev|first1=Igor D.|last2=Makarova|first2=Lidia N.|last3=Brent Tully|first3=R.|last4=Anand|first4=Gagandeep S.|last5=Rizzi|first5=Luca|last6=Shaya|first6=Edward J.|last7=Afanasiev|first7=Viktor L.|s2cid=218538458|journal=Astronomy & Astrophysics|volume=638|pages=A111|arxiv=2005.03132|bibcode=2020A&A...638A.111K}}</ref> Note that Karachentsev divides this group into two subgroups centered around [[IC 342]] and [[Maffei 1]].
 
{| class="wikitable" style="text-align:center;border-collapse:collapse;" cellpadding="2"
|+'''Members of the IC 342 Subgroup'''
|-
! style="background:#efefef;" | Name
! style="background:#efefef;" | [[Galaxy morphological classification|Type]]<ref name="ned">{{cite web
  | title=NASA/IPAC Extragalactic Database
  | work=Results for various galaxies
  | url=http://nedwww.ipac.caltech.edu/
  | access-date=2006-12-30}}</ref>
! style="background:#efefef;" | [[Right ascension|R.A.]] ([[Epoch (astronomy)#Julian years and J2000|J2000]])<ref name="ned" />
! style="background:#efefef;" | [[Declination|Dec.]] ([[Epoch (astronomy)#Julian years and J2000|J2000]])<ref name="ned" />
! style="background:#efefef;" | [[Redshift]] (km/[[second|s]])<ref name="ned" />
! style="background:#efefef;" | [[Apparent magnitude|Apparent Magnitude]]<ref name="ned" />
|- 
| [[Camelopardalis A]]
| Irr
| {{RA|04|26|16.3}}
| {{DEC|+72|48|21}}
| –46 ± 1
| 14.8
|- 
| [[Camelopardalis B]]
| Irr
| {{RA|04|53|07.1}}
| {{DEC|+67|05|57}}
| 77
| 16.1
|- 
| [[IC 342]]
| SAB(rs)cd
| {{RA|03|46|48.5}}
| {{DEC|+68|05|46}}
| 31 ± 3
| 9.1
|- 
| [[KK 35]]
| Irr
| {{RA|03|45|12.6}}
| {{DEC|+67|51|51}}
| 105 ± 1
| 17.2
|- 
| [[KKH 22]]<ref name=Karachentsev2020/>
| dSph
| {{RA|03|44|56.6}}
| {{DEC|+72|03|52}}
| 30 ±&nbsp;10
| 15.3
|- 
| [[NGC 1560]]
| SA(s)d
| {{RA|04|32|49.1}}
| {{DEC|+71|52|59}}
| –36 ± 5
| 12.2
|- 
| [[NGC 1569]]
| Sbrst	
| {{RA|04|30|49.1}}	
| {{DEC|+64|50|52,6}}
| –104 ± 4
| 11.2
|-
| [[UGCA 86]]
| Im
| {{RA|03|59|50.5}}
| {{DEC|+67|08|37}}
| 67 ± 4
| 13.5
|- 
| [[UGCA 92]]
| Im
| {{RA|04|32|04.9}}
| {{DEC|+63|36|49.0}}
| –99 ± 5
| 13.8
|-
| [[UGCA 105]]
| Im
| {{RA|05|14|15.3}}
| {{DEC|+62|34|48}}
| 111 ± 5
| 13.9
|-
|}

{| class="wikitable" style="text-align:center;border-collapse:collapse;" cellpadding="2"
|+'''Members of the Maffei 1 Subgroup'''
|-
! style="background:#efefef;" | Name
! style="background:#efefef;" | [[Galaxy morphological classification|Type]]<ref name="ned" />
! style="background:#efefef;" | [[Right ascension|R.A.]] ([[Epoch (astronomy)#Julian years and J2000|J2000]])<ref name="ned" />
! style="background:#efefef;" | [[Declination|Dec.]] ([[Epoch (astronomy)#Julian years and J2000|J2000]])<ref name="ned" />
! style="background:#efefef;" | [[Redshift]] (km/[[second|s]])<ref name="ned" />
! style="background:#efefef;" | [[Apparent magnitude|Apparent Magnitude]]<ref name="ned" />
|- 
| [[Dwingeloo 1]]
| SB(s)cd
| {{RA|02|56|51.9}}
| {{DEC|+58|54|42}}
| 110
| 8.3
|- 
| [[Dwingeloo 2]]
| Im
| {{RA|02|54|08.5}}
| {{DEC|+59|00|19}}
| 94 ± 1
| 20.5
|- 
| [[KKH 11]]
| dE
| {{RA|02|24|34.2}}
| {{DEC|+56|00|43}}
| 310
| 16.2
|- 
| [[KKH 12]]
| Irr
| {{RA|02|27|26.9}}
| {{DEC|+57|29|16}}
| 70
| 17.8
|- 
| [[Maffei 1]]
| S0 pec
| {{RA|02|36|35.4}}
| {{DEC|+59|39|19}}
| 13 ± 22
| 11.4
|- 
| [[Maffei 2]]
| SAB(rs)bc
| {{RA|02|41|55.1}}
| {{DEC|+59|36|15}}
| –17 ± 5
| 16.0
|- 
| [[MB 1]]
| SAB(s)d
| {{RA|02|35|36.5}}
| {{DEC|+59|22|43}}
| 190 ± 1
| 20.5
|- 
| [[MB 3]]
| dSph
| {{RA|02|55|42.7}}
| {{DEC|+58|51|37}}
| 59 ± 1
| 17.33
|-
|}

Additionally, [[KKH 37]] is listed as possibly being a member of the IC 342 Subgroup, and [[KKH 6]] is listed as possibly being a member of the Maffei 1 Subgroup.<ref name="karachentsev2005" />

{{Wide image|Maffei 1 and 2.jpg|650px|Maffei 1 and Maffei 2 are visible in this image.}}