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Dragonfly 44 is an ultra diffuse galaxy in the Coma Cluster.[1][3][2][4] This galaxy is well-known because observations of the velocity dispersion in 2016 suggested a mass of about one trillion solar masses, about the same as the Milky Way. This mass was consistent with a count of about 90 and 70 globular clusters observed around Dragonfly 44 in two different studies.

Dragonfly 44
Hubble Space Telescope view of the galaxy Dragonfly 44
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension13h 00m 58.0s[1]
Declination+26° 58′ 35″[1]
Redshift~0.023
Helio radial velocity6280 ± 120 km/s
Distance~100 Mpc (~330 Mly)
Group or clusterComa Cluster
Apparent magnitude (V)21 mags; or 19.4 mags [2]
Apparent magnitude (B)22
Absolute magnitude (V)-16.1 mag [2]
Characteristics
Mass~1.6×1011 M☉
Apparent size (V)10 x 35 arcsec
Other designations
SDSS J130057.98+265839.6, SDSS J130058.17+265836.1, SDSS J130058.21+265829.3

Later, spatially resolved kinematics measured a mass of about 160 billion solar masses, six times less than early mass measurements and 1 order of magnitude less than the Milky Way's mass.[5] The most recent work found 20 globular clusters around the galaxy, which is consistent with the current mass measurement.[6][7] The lack of X-ray emission from the universe and surroundings also show that the number of globular clusters cannot be as many as was claimed before.[8]

The galaxy emits only 1% of the light emitted by the Milky Way.[9] The galaxy was discovered with the Dragonfly Telephoto Array.[10]


Early study


To determine the amount of dark matter in this galaxy, in 2016, astronomers used the DEIMOS instrument installed on Keck II to measure the velocities of stars for 33.5 hours for six nights so they could determine the galaxy's mass. The scientists then used the Gemini Multi-Object Spectrograph on the 8-m Gemini North telescope to reveal a halo of spherical clusters of stars around the galaxy's core.[11] Following this observation, in August 2016, astronomers reported that this galaxy might be made almost entirely of dark matter.[12][13][14]


See also



References


  1. Van Dokkum, Pieter; et al. (7 January 2015). "Forty-Seven Milky Way-sized, Extremely Diffuse Galaxies in the Coma-Cluster". The Astrophysical Journal Letters. 798 (2): L45. arXiv:1410.8141. Bibcode:2015ApJ...798L..45V. doi:10.1088/2041-8205/798/2/L45. S2CID 119279968.
  2. Van Dokkum, Pieter; et al. (1 May 2015). "Spectroscopic confirmation of the existence of large, diffuse galaxies in the coma cluster". The Astrophysical Journal Letters. 804 (1): L26. arXiv:1504.03320. Bibcode:2015ApJ...804L..26V. doi:10.1088/2041-8205/804/1/L26. S2CID 54664026.
  3. "Scientists discover the fluffiest galaxies". phys.org. 14 May 2015.
  4. Dragonfly 44: Ultra-Diffuse Galaxy Made Mostly of Dark Matter. Aug 2016
  5. Van Dokkum, Pieter; Wasserman, Asher; Danieli, Shany; Abraham, Roberto; Brodie, Jean; Conroy, Charlie; Forbes, Duncan A.; Martin, Christopher; Matuszewski, Matt; Romanowsky, Aaron J.; Villaume, Alexa (2019). "Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. I. Observations, Kinematics, and Cold Dark Matter Halo Fits, Peter van Dokkum et al. 2019". The Astrophysical Journal. 880 (2): 91. arXiv:1904.04838. doi:10.3847/1538-4357/ab2914. S2CID 119185644.
  6. Saifollahi, Teymoor; Trujillo, Ignacio; Beasley, Michael A.; Peletier, Reynier F.; Knapen, Johan H. (2020). ""The number of globular clusters around the iconic UDG DF44 is as expected for dwarf galaxies", Saifollahi et al. 2020". Monthly Notices of the Royal Astronomical Society. 502 (4): 5921–5934. arXiv:2006.14630. doi:10.1093/mnras/staa3016. S2CID 220127887.
  7. "The puzzle of the strange galaxy made of 99.99% dark matter is solved".
  8. Bogdan, Akos (2020). ""The American Astronomical Society, find out more The Institute of Physics, find out more The Archetypal Ultra-diffuse Galaxy, Dragonfly 44, Is not a Dark Milky Way", Bogdan 2020". The Astrophysical Journal Letters. arXiv:2009.07846. doi:10.3847/2041-8213/abb886. S2CID 221761669.
  9. Crosswell, Ken (26 July 2016). "The Milky Way's dark twin revealed". Nature News. Retrieved 30 July 2016.
  10. Rachel Feltman (25 August 2016). "A new class of galaxy has been discovered, one made almost entirely of dark matter". The Washington Post.
  11. "A galaxy made of 99.9% dark matter | Space | EarthSky". 30 August 2016.
  12. Van Dokkum, Pieter; et al. (25 August 2016). "A High Stellar Velocity Dispersion and ~100 Globular Clusters For The Ultra-Diffuse Galaxy Dragonfly 44". The Astrophysical Journal Letters. 828 (1): L6. arXiv:1606.06291. Bibcode:2016ApJ...828L...6V. doi:10.3847/2041-8205/828/1/L6. S2CID 1275440.
  13. Hall, Shannon (25 August 2016). "Ghost galaxy is 99.99 per cent dark matter with almost no stars". New Scientist. Retrieved 27 August 2016.
  14. Feltman, Rachael (26 August 2016). "A new class of galaxy has been discovered, one made almost entirely of dark matter". The Washington Post. Retrieved 26 August 2016.


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На других языках

[de] Dragonfly 44

Dragonfly 44 (deutsch Libelle 44) ist eine Galaxie mit einem sehr hohen Anteil an Dunkler Materie.[4][5] Sie ist ein Beispiel für eine ultra-diffuse Galaxie im Coma-Galaxienhaufen.[6][7] Die gemessene Rotationsgeschwindigkeit legt eine Masse von einer Billion Sonnenmassen nahe, was der Masse der Milchstraße entspricht. Aber die Lichtemission der Galaxie beträgt nur ca. 1 % der Lichtemission der Milchstraße.[8]
- [en] Dragonfly 44

[ru] Dragonfly 44

Dragonfly 44 — тусклая массивная галактика в скоплении Волос Вероники с массой в один триллион солнечных масс, что сопоставимо с массой Млечного Пути. Обладая крайне малым для такой массы количеством звёзд и низкой звёздной плотностью, считается почти полностью (на 99,99 %) состоящей из тёмной материи.


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