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NGC 604

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NGC604
Emission nebula
H II region
NGC 604 inside theTriangulum Galaxy
(viewed by theJames Webb Space Telescope)
Observation data:J2000epoch
Right ascension01h34m33.2s[1]
Declination+30° 47′ 06″[1]
Distance2,700,000ly(840,000[2]pc)
Apparent magnitude(V)+14.0[1]
Apparent dimensions (V)1.93x 1.2arcmins[1]
ConstellationTriangulum
Physical characteristics
Radius760[3]ly
Absolute magnitude(V)-13.8
Notable featuresmassiveH II region
3.5 million years old[2]
See also:Lists of nebulae

NGC 604is anH II regioninside theTriangulum Galaxy.It was discovered byWilliam Herschelon September 11, 1784. It is among thelargest H II regionsin theLocal Groupof galaxies; at the galaxy's estimated distance of 2.7 millionlight-years,its longest diameter is roughly 1,520 light years (~460parsecs), over 40 times the size of the visible portion of theOrion Nebula.It is over 6,300 times moreluminousthan theOrion Nebula,and if it were at the same distance it would outshineVenus.Its gas isionizedby a cluster of massivestarsat its center[4]with 200 stars of spectral typeOandWR,a mass of 105solar masses,and an age of 3.5 million years;[2]however, unlike theLarge Magellanic Cloud'sTarantula Nebulacentral cluster (R136), NGC 604's one is much less compact and more similar to a largestellar association.[5]

See also

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References

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  1. ^abcd"NASA/IPAC Extragalactic Database".Results for NGC 604.Retrieved2006-09-03.
  2. ^abcBarba, Rodolfo (2004). "An in-depth analysis of a prototypical giant H II region: NGC 604".HST Proposal ID #10419:10419.Bibcode:2004hst..prop10419B.
  3. ^distance × sin( diameter_angle / 2 ) = 760 ly. radius
  4. ^Nemiroff, R.; Bonnell, J., eds. (2 November 2002)."NGC 604: Giant Stellar Nursery".Astronomy Picture of the Day.NASA.
  5. ^Maíz-Apellániz, J.; Pérez, E.; Mas-Hesse, J. M. (2004). "NGC 604, the Scaled OB Association (SOBA) Prototype. I. Spatial Distribution of the Different Gas Phases and Attenuation by Dust".The Astronomical Journal.128(3): 1196–1218.arXiv:astro-ph/0406130.Bibcode:2004AJ....128.1196M.doi:10.1086/422925.S2CID8099926.
  • Some data in the table was updated from Sue French's column "Deep-sky Wonders", in the January 2006 issue ofSky & Telescope,p. 83.
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