IC 342/Maffei Group explained

The IC 342/Maffei Group (also known as the IC 342 Group or the Maffei 1 Group) corresponds to one or two galaxy groups close to the Local Group. The member galaxies are mostly concentrated around either IC 342 or Maffei 1, which would be the brightest two galaxies in the group.[1] The group is part of the Virgo Supercluster.[2] However, recent studies have found that the two subgroups are unrelated; while the IC 342 group is the nearest galaxy group to the Milky Way, the Maffei 1 group is several times farther away, and is not gravitationally bound to the IC 342 group.[3] [4]

Members

The table below lists galaxies that have been identified as associated with the IC342/Maffei 1 Group by I. D. Karachentsev.[5] Note that Karachentsev divides this group into two subgroups centered around IC 342 and Maffei 1.

Members of the IC 342 Subgroup
NameType[6] R.A. (J2000)Dec. (J2000)Redshift (km/s)Apparent Magnitude
Camelopardalis AIrr–46 ± 114.8
Camelopardalis BIrr7716.1
IC 342SAB(rs)cd31 ± 39.1
KK 35Irr105 ± 117.2
KKH 22dSph30 ± 1015.3
NGC 1560SA(s)d–36 ± 512.2
NGC 1569Sbrst –104 ± 411.2
UGCA 86Im67 ± 413.5
UGCA 92Im–99 ± 513.8
UGCA 105Im111 ± 513.9
Members of the Maffei 1 Subgroup
NameTypeR.A. (J2000)Dec. (J2000)Redshift (km/s)Apparent Magnitude
Dwingeloo 1SB(s)cd1108.3
Dwingeloo 2Im94 ± 120.5
KKH 11dE31016.2
KKH 12Irr7017.8
Maffei 1S0 pec13 ± 2211.4
Maffei 2SAB(rs)bc–17 ± 516.0
MB 1SAB(s)d190 ± 120.5
MB 3dSph59 ± 117.33

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.

Foreground dust obscuration

As seen from Earth, the group lies near the plane of the Milky Way (a region sometimes called the Zone of Avoidance). Consequently, the light from many of the galaxies is severely affected by dust obscuration within the Milky Way. This complicates observational studies of the group, as uncertainties in the dust obscuration also affect measurements of the galaxies' luminosities and distances as well as other related quantities.[7]

Moreover, the galaxies within the group have historically been difficult to identify. Many galaxies have only been discovered using late 20th century astronomical instrumentation. For example, Maffei 1 and Maffei 2 were only discovered in 1968 using infrared photographic images of the region.[8] Furthermore, it is difficult to determine whether some objects near IC 342 or Maffei 1 are galaxies associated with the IC 342/Maffei Group or diffuse foreground objects within the Milky Way that merely look like galaxies. For example, the objects MB 2 and Camelopardalis C were once thought to be dwarf galaxies in the IC 342/Maffei Group but are now known to be objects within the Milky Way.[9]

Group formation and possible interactions with the Local Group

Since the IC 342/Maffei Group and the Local Group are located physically close to each other, the two groups may have influenced each other's evolution during the early stages of galaxy formation. An analysis of the velocities and distances to the IC 342/Maffei Group as measured by M. J. Valtonen and collaborators suggested that IC 342 and Maffei 1 were moving faster than what could be accounted for in the expansion of the universe. They therefore suggested that IC 342 and Maffei 1 were ejected from the Local Group after a violent gravitational interaction with the Andromeda Galaxy during the early stages of the formation of the two groups.[10]

However, this interpretation is dependent on the distances measured to the galaxies in the group, which in turn is dependent on accurately measuring the degree to which interstellar dust in the Milky Way obscures the group.[11] More recent observations have demonstrated that the dust obscuration may have been previously overestimated, so the distances may have been underestimated. If these new distance measurements are correct, then the galaxies in the IC 342/Maffei Group appear to be moving at the rate expected from the expansion of the universe, and the scenario of a collision between the IC 342/Maffei Group and the Local Group would be implausible.

Notes and References

  1. I. D. Karachentsev . The Local Group and Other Neighboring Galaxy Groups . Astronomical Journal . 2005 . 129 . 1 . 178–188 . 2005AJ....129..178K . 10.1086/426368. astro-ph/0410065 . 119385141 .
  2. R. B. Tully . The Local Supercluster . Astrophysical Journal . 1982 . 257 . 389–422 . 1982ApJ...257..389T . 10.1086/159999. free .
  3. 10.1134/S1990341318030021. Does the IC 342/Maffei Galaxy Group Really Exist?. 2018. Tikhonov. N. A.. Galazutdinova. O. A.. Astrophysical Bulletin. 73. 3. 279–292. 2018AstBu..73..279T. 126018966.
  4. 10.3847/2041-8213/aafee6. The Distance and Motion of the Maffei Group. 2019. Anand. Gagandeep S.. Tully. R. Brent. Rizzi. Luca. Karachentsev. Igor D.. The Astrophysical Journal. 872. 1. L4. 1901.05981. 2019ApJ...872L...4A. 119227716 . free .
  5. 10.1051/0004-6361/202037993. KKH 22, the first dwarf spheroidal satellite of IC 342. 2020. Karachentsev. Igor D.. Makarova. Lidia N.. Brent Tully. R.. Anand. Gagandeep S.. Rizzi. Luca. Shaya. Edward J.. Afanasiev. Viktor L.. 218538458. Astronomy & Astrophysics. 638. A111. 2005.03132. 2020A&A...638A.111K.
  6. Web site: NASA/IPAC Extragalactic Database . Results for various galaxies . 2006-12-30.
  7. R. J. Buta . M. L. McCall . The IC 342/Maffei Group Revealed . Astrophysical Journal Supplement Series . 1999 . 124 . 1 . 33–93 . 1999ApJS..124...33B . 10.1086/313255. free .
  8. P. Maffei . Infrared Object in the Region of IC 1895 . Publications of the Astronomical Society of the Pacific . 1968 . 80 . 476 . 618–621 . 1968PASP...80..618M . 10.1086/128698. free .
  9. I. D. Karachentsev . M. E. Sharina . A. E. Dolphin . E. K. Grebel . Distances to nearby galaxies around IC 342 . Astronomy and Astrophysics . 2003 . 408 . 1 . 111–118 . 2003A&A...408..111K . 10.1051/0004-6361:20030912. free.
  10. M. J. Valtonen . G. G. Byrd . M. L. McCall . K. A. Innanen . A revised history of the Local Group and a generalized method of timing . Astronomical Journal . 1993 . 105 . 886–893 . 1993AJ....105..886V . 10.1086/116480.
  11. R. L. Fingerhut . H. Lee . M. L. McCall . M. G. Richer . The Extinction and Distance of Maffei 2 and a New View of the IC 342/Maffei Group . 2007 . Astrophysical Journal . 655 . 2 . 814–830 . astro-ph/0610044. 2007ApJ...655..814F . 10.1086/509862 . 18405597 .