Holmberg II

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search
Holmberg II
File:Irregular galaxy Holmberg II (captured by the Hubble Space Telescope).tif
An image of Holmberg II, NASA/JPL-Caltech/K. Gordon (STScI), SINGS
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension08h 19m 04.98s [1]
Declination+70° 43′ 12.1″[1]
Redshift0.000474 ± 0.000003[1]
Heliocentric radial velocity142±1[1]
Distance11.06 Mly
Apparent magnitude (V)11.10[1]
Characteristics
TypeIm [1]
Apparent size (V)7′.9 × 6′.3[1]
Other designations
UGC 4305, PGC 23324, MCG +12-8-33, IRAS 08140+7052, Arp 268, DDO 50, Holmberg II, KUG 0814+708[1]

Holmberg II is an irregular dwarf galaxy in the constellation Ursa Major. Its apparent magnitude is 11,1m and it is 11 million light years away from Earth. The galaxy is dominated by huge glowing gas bubbles, which are regions of star formation.[2][3]

Holmberg II also hosts an ultraluminous X-ray source. One hypothesis suggests that is caused by an intermediate mass black hole that is pulling surrounding material.[2] Holmberg II was discovered by Erik Bertil Holmberg.

References

[edit | edit source]
  1. ^ a b c d e f g h Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  2. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  3. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
[edit | edit source]
  • Error creating thumbnail: File missing Media related to Lua error in Module:Commons_link at line 62: attempt to index field 'wikibase' (a nil value). at Wikimedia Commons