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IC 342/Maffei Group
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==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' [[luminosity|luminosities]] and distances as well as other related quantities.<ref name="karachentsev2005" /><ref name="butamccall1999">{{cite journal |author1=R. J. Buta |author2=M. L. McCall | title=The IC 342/Maffei Group Revealed | journal=Astrophysical Journal Supplement Series | date=1999 | volume=124 | issue= 1 | pages=33β93 | bibcode=1999ApJS..124...33B | doi = 10.1086/313255 | doi-access=free }}</ref> 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.<ref name="maffei1968">{{cite journal | author= P. Maffei | title=Infrared Object in the Region of IC 1895 | journal=Publications of the Astronomical Society of the Pacific | date=1968 | volume=80 | issue=476 | pages=618β621 | bibcode=1968PASP...80..618M | doi = 10.1086/128698 | doi-access=free }}</ref> 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]].<ref name="karachentsevetal2003">{{cite journal |author1=I. D. Karachentsev |author2=M. E. Sharina |author3=A. E. Dolphin |author4=E. K. Grebel | title=Distances to nearby galaxies around IC 342 | journal=Astronomy and Astrophysics | date=2003 | volume=408 | issue= 1 | pages=111β118 | bibcode=2003A&A...408..111K | doi = 10.1051/0004-6361:20030912 | doi-access=free}}</ref>
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