IC 342/Maffei Group

The IC 342/Maffei Group (also known as the IC 342 Group or the Maffei 1 Group) is the nearest group of galaxies to the Local Group. The group can be described as a binary group; the member galaxies are mostly concentrated around either IC 342 or Maffei 1, both of which are the brightest galaxies within the group.[1] The group is part of the Virgo Supercluster.[2]

IC 342/Maffei Group
Maffei 1, one of the brightest galaxies in the group
Observation data (Epoch J2000)
Constellation(s)	Cassiopeia/Camelopardalis/Perseus
Brightest member	IC 342[1]
Number of galaxies	16[1]
Other designations
IC 342 Group, Maffei 1 Group, LGG 104

Members

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

Members of the IC 342 Subgroup

Name	Type[3]	R.A. (J2000)[3]	Dec. (J2000)[3]	Redshift (km/s)[3]	Apparent Magnitude[3]
Camelopardalis A	Irr	04^h 26^m 16.3^s	+72° 48′ 21″	-46 ± 1	14.8
Camelopardalis B	Irr	04^h 53^m 07.1^s	+67° 05′ 57″	77	16.1
Cassiopeia 1	dIrr	02^h 06^m 02.8^s	+68° 59′ 59″	35	16.4
IC 342	SAB(rs)cd	03^h 46^m 48.5^s	+68° 05′ 46″	31 ± 3	9.1
KK 35	Irr	03^h 45^m 12.6^s	+67° 51′ 51″	105 ± 1	17.2
NGC 1560	SA(s)d	04^h 32^m 49.1^s	+71° 52′ 59″	-36 ± 5	12.2
NGC 1569	Sbrst	04^h 30^m 49.1^s	+64° 50′ 52,6″	-104 ± 4	11.2
UGCA 86	Im	03^h 59^m 50.5^s	+67° 08′ 37″	67 ± 4	13.5
UGCA 92	Im	04^h 32^m 04.9^s	+63° 36′ 49.0″	-99 ± 5	13.8
UGCA 105	Im	05^h 14^m 15.3^s	+62° 34′ 48″	111 ± 5	13.9

Members of the Maffei 1 Subgroup

Name	Type[3]	R.A. (J2000)[3]	Dec. (J2000)[3]	Redshift (km/s)[3]	Apparent Magnitude[3]
Dwingeloo 1	SB(s)cd	02^h 56^m 51.9^s	+58° 54′ 42″	110	8.3
Dwingeloo 2	Im	02^h 54^m 08.5^s	+59° 00′ 19″	94 ± 1	20.5
KKH 11	dE	02^h 24^m 34.2^s	+56° 00′ 43″	310	16.2
KKH 12	Irr	02^h 27^m 26.9^s	+57° 29′ 16″	70	17.8
Maffei 1	S0 pec	02^h 36^m 35.4^s	+59° 39′ 19″	13 ± 22	11.4
Maffei 2	SAB(rs)bc	02^h 41^m 55.1^s	+59° 36′ 15″	-17 ± 5	16.0
MB 1	SAB(s)d	02^h 35^m 36.5^s	+59° 22′ 43″	190 ± 1	20.5
MB 3	dSph	02^h 55^m 42.7^s	+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.[1]

Maffei 1 and Maffei 2 are visible in this image.

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.[1][4]

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, while many fainter, more distant galaxies, such as the galaxies in the New General Catalogue, were already identified visually by the end of the nineteenth century, Maffei 1 and Maffei 2 were only discovered in 1968 using infrared photographic images of the region.[5] 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.[6]

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.[7]

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.[4][8] 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.[8]

References

1. I. D. Karachentsev (2005). "The Local Group and Other Neighboring Galaxy Groups". Astronomical Journal. 129 (1): 178–188. arXiv:astro-ph/0410065. Bibcode:2005AJ....129..178K. doi:10.1086/426368.
2. R. B. Tully (1982). "The Local Supercluster". Astrophysical Journal. 257: 389–422. Bibcode:1982ApJ...257..389T. doi:10.1086/159999.
3. "NASA/IPAC Extragalactic Database". Results for various galaxies. Retrieved 2006-12-30.
4. R. J. Buta; M. L. McCall (1999). "The IC 342/Maffei Group Revealed". Astrophysical Journal Supplement Series. 124 (1): 33–93. Bibcode:1999ApJS..124...33B. doi:10.1086/313255.
5. P. Maffei (1968). "Infrared Object in the Region of IC 1895". Publications of the Astronomical Society of the Pacific. 80 (476): 618–621. Bibcode:1968PASP...80..618M. doi:10.1086/128698.
6. I. D. Karachentsev; M. E. Sharina; A. E. Dolphin; E. K. Grebel (2003). "Distances to nearby galaxies around IC 342". Astronomy and Astrophysics. 408 (1): 111–118. Bibcode:2003A&A...408..111K. doi:10.1051/0004-6361:20030912.
7. M. J. Valtonen; G. G. Byrd; M. L. McCall; K. A. Innanen (1993). "A revised history of the Local Group and a generalized method of timing". Astronomical Journal. 105: 886–893. Bibcode:1993AJ....105..886V. doi:10.1086/116480.
8. R. L. Fingerhut; H. Lee; M. L. McCall; M. G. Richer (2007). "The Extinction and Distance of Maffei 2 and a New View of the IC 342/Maffei Group". Astrophysical Journal. 655 (2): 814–830. arXiv:astro-ph/0610044. Bibcode:2007ApJ...655..814F. doi:10.1086/509862.

External links