Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
IC 342/Maffei Group
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==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>
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
IC 342/Maffei Group
(section)
Add topic