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MACS J0416.1-2403

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MACS J0416.1–2403
Galaxy cluster MCS J0416.1–2403 imaged by theHubble Space Telescope
Observation data (EpochJ2000.0[1])
Constellation(s)Eridanus
Right ascension04h16m09.9s[1]
Declination−24° 03′ 58″[1]
Redshift0.420000[1]
Other designations
MACSJ0416.1-2403,[1]MACS J0416-2403, MACS 0416.1-2403, MACS 0416-2403, 1RXS J041609.9-240358[1]

MACS J0416.1-2403or MACS0416 abbreviated, is acluster of galaxiesat aredshiftof z=0.397 with a mass 160 trillion times themass of the Suninside 200kpc(650kly). Its mass extends out to a radius of 950 kpc (3,100 kly) and was measured as 1.15 × 1015solar masses.[2]The system was discovered[3]in images taken by theHubble Space Telescopeduring theMassive Cluster Survey,MACS.[4]This cluster causesgravitational lensingof distant galaxies producing multiple images.[5][6]Based on the distribution of the multiple image copies, scientists have been able to deduce and map the distribution ofdark matter.[7][8]The images, released in 2014,[9]were used in theCluster Lensing And Supernova survey with Hubble (CLASH)to help scientists peer back in time at the early Universe and to discover the distribution of dark matter.[10]

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See also

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Mothra (star)

References

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  1. ^abcdef"Object No. 1 - MACS J0416.1-2403".NASA/IPAC Extragalactic Database.
  2. ^Jauzac, Mathilde; Eric Jullo; Dominique Eckert; Harald Ebeling; Johan Richard; Marceau Limousin; et al. (23 June 2014)."Hubble Frontier Fields: The Geometry and Dynamics of the Massive Galaxy Cluster Merger MACSJ0416.1-2403".Monthly Notices of the Royal Astronomical Society.446(4): 4132–4147.arXiv:1406.3011.Bibcode:2015MNRAS.446.4132J.doi:10.1093/mnras/stu2425.
  3. ^Mann, Andrew; Harald Ebeling (March 2012)."X-ray-optical classification of cluster mergers and the evolution of the cluster merger fraction".Monthly Notices of the Royal Astronomical Society.420(3): 2120–2138.arXiv:1111.2396.Bibcode:2012MNRAS.420.2120M.doi:10.1111/j.1365-2966.2011.20170.x.S2CID118744581.
  4. ^Ebeling, Harald; Alastair Edge; J. Patrick Henry (June 2001). "MACS: A Quest for the Most Massive Galaxy Clusters in the Universe".The Astrophysical Journal.553(2): 668–676.arXiv:astro-ph/0009101.Bibcode:2001ApJ...553..668E.doi:10.1086/320958.S2CID15324781.
  5. ^Diego, Jose M. (4 June 2014)."Free Form Lensing Implications for the Collision of Dark Matter and Gas in the Frontier Fields Cluster MACSJ0416.1-2403".Monthly Notices of the Royal Astronomical Society.447(4): 3130–3149.arXiv:1406.1217.Bibcode:2015MNRAS.447.3130D.doi:10.1093/mnras/stu2660.
  6. ^"New mass map of a distant galaxy cluster is the most precise yet".24 July 2014.Retrieved25 July2014.
  7. ^Cho, Adrian (2017)."Scientists unveil the most detailed map of dark matter to date".Science.doi:10.1126/science.aal0847.
  8. ^Natarajan, Priyamvada; Chadayammuri, Urmila; Jauzac, Mathilde; Richard, Johan; Kneib, Jean-Paul; Ebeling, Harald; Jiang, Fangzhou; Bosch, Frank van den; Limousin, Marceau; Jullo, Eric; Atek, Hakim; Pillepich, Annalisa; Popa, Cristina; Marinacci, Federico; Hernquist, Lars; Meneghetti, Massimo; Vogelsberger, Mark (2017)."Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations".Monthly Notices of the Royal Astronomical Society.468(2): 1962–1980.arXiv:1702.04348.Bibcode:2017MNRAS.468.1962N.doi:10.1093/mnras/stw3385.
  9. ^"New mass map of a distant galaxy cluster is the most precise yet".24 July 2014.
  10. ^"Cluster Lensing And Supernova survey with Hubble (CLASH)".23 June 2017.
  11. ^"A cosmic kaleidoscope".Retrieved23 March2016.
  12. ^"Faint Compact Galaxy in the Early Universe".Retrieved22 December2015.
  13. ^"Hubble Frontier Fields view of MACSJ0416.1–2403".Retrieved23 October2015.