An ultra diffuse galaxy (UDG), or Dark galaxy,[1] is an extremely low luminosity
galaxy, the first example of which was discovered in the nearby
Virgo Cluster by
Allan Sandage and Bruno Binggeli in 1984.[a] These galaxies have been studied for many years prior to their renaming in 2015. Their lack of luminosity is due to the lack of star-forming gas, which results in these galaxies being reservoirs of very old stellar populations.[3][4]
Based on discoveries confirmed in 2018, this class of galaxies includes both extremes of
dark matter content: Some UDGs consist almost entirely of dark matter (such a galaxy may have the same size and mass as the
Milky Way but a visible star count of only 1%),[5] while other UDGs appear to be almost entirely free of dark matter.[6]
Examples
Some ultra diffuse galaxies found in the
Coma Cluster, about 330 million light years from Earth, have diameters of 60
kly (18
kpc) with 1% of the stars of the
Milky Way Galaxy.[7] The distribution of ultra diffuse galaxies in the Coma Cluster is the same as luminous galaxies; this suggests that the cluster environment strips the gas from the galaxies, while allowing them to populate the cluster the same as more luminous galaxies. The similar distribution in the higher tidal force zones suggests a larger dark matter fraction to hold the galaxies together under the higher stress.[3]
Dragonfly 44, an ultra diffuse galaxy in the
Coma Cluster, is one example.[4] Observations of its rotational speed suggest a mass of about one trillion
solar masses, about the same as the mass of the
Milky Way. This is also consistent with about 90
globular clusters observed around
Dragonfly 44. However, the galaxy emits only 1% of the light emitted by the Milky Way.[8] On 25 August 2016, astronomers reported that
Dragonfly 44 may be made almost entirely of
dark matter.[9][5][10] However, later, spatially resolved kinematics measured a mass of about 160 billion solar mass, six times less than early mass measurements and 1 order of magnitude less than the
Milky Way mass.[11] The most recent work found 20
globular clusters around the galaxy, which is consistent with the recent mass measurement.[12][13] The lack of X-ray emissions from the galaxy and surrounding area also show that the number of
globular clusters can not be as many as was claimed before.[14]
In 2021, AGC 114905, an ultra-diffuse dwarf galaxy about 250 million light-years away, was reported to have almost no dark matter.[18] However, this conclusion relies heavily on the galaxy having a moderate inclination of 32° between disc and sky planes, which is estimated from the somewhat oval appearance. Using detailed simulations of AGC 114905 in the alternative gravity theory known as
Modified Newtonian Dynamics, it was shown that a disc galaxy with its properties can appear slightly oval even if viewed face-on due to disc self-gravity, in which case the rotation curve could be much higher and the galaxy could be quite consistent with theoretical expectations.[19] An overestimated inclination is unlikely if galaxies are dominated by dark matter because then the disc is not self-gravitating, so it should be close to circular when viewed face-on.[20]
See also
Dark galaxy – A hypothesized galaxy with no, or very few, stars
Low-surface-brightness galaxy, also known as LSBG – Galaxy which is less bright than the ambient night skyPages displaying short descriptions of redirect targets
Type-cD galaxy – Galaxy morphology classification or c-Diffuse galaxy type
Type-D galaxy – System for categorizing galaxies based on appearancePages displaying short descriptions of redirect targets or Diffuse-type galaxy
DGSAT I – Ultra diffuse galaxy in the Perseus–Pisces Supercluster
Footnotes
^UDGs are a subset of dwarf spheroidals and dwarf ellipticals and as such are a redundant name for an already well studied galaxy type.[2]
^NGC 1052-DF2 had previously been identified on photographic plates by Karachentsev et al. in 2000.[15]
van Dokkum, Pieter G.; Romanowsky, Aaron J.; Abraham, Roberto; Brodie, Jean P.; Conroy, Charlie;
Geha, Marla; Merritt, Allison; Villaume, Alexa; Zhang, Jielai (6 February 2015). "Spectroscopic confirmation of the existence of large, diffuse galaxies in the Coma cluster". The Astrophysical Journal Letters. 804 (1) (published 1 May 2015): L26.
arXiv:1504.03320.
Bibcode:
2015ApJ...804L..26V.
doi:
10.1088/2041-8205/804/1/L26.
S2CID54664026.