词条 | NGC 2070 |
释义 |
| name = NGC 2070 | image = | caption = ESO image of the 30 Doradus nebula | credit = ESO/IDA/Danish 1.5 m/R. Gendler, C. C. Thöne, C. Féron, and J.-E. Ovaldsen | epoch = J2000 | constellation = | ra = {{RA|05|38|42}}[1] | dec = {{DEC|-69|06|00}}[1] | dist_ly = 157 kly | dist_pc = 48.5 kpc | appmag_v = 7.25[1] | size_v = 3.50′ × 3.50′ | age = | notes = | names = Caldwell 103 PKS 0539-69 }}NGC 2070 is a large open cluster and candidate super star cluster located on the south-east corner of the Large Magellanic Cloud.[2] It is located at the centre of the Tarantula Nebula and produces most of the energy that makes it visible. Its central condensation is the star cluster R136, one of the most energetic star clusters known.[3] It holds a number of massive stars, including the most massive star known, R136a1, at 315 {{Solar mass}} and 8.7 million {{Solar luminosity}}.[4] References1. ^1 2 {{cite simbad|title=NGC 2070|accessdate=11 August 2017}} 2. ^{{cite journal|bibcode=1963IrAJ....6...74S|title=A Catalogue of Clusters in The LMC|journal=Irish Astronomical Journal|volume=6|pages=74|language=en|last1=Shapley|first1=H.|last2=Lindsay|first2= E. M.|year=1963}} 3. ^{{cite journal | last=Bosch | first=Guillermo |author2=Terlevich, Elena |author3=Terlevich, Roberto | title=Gemini/GMOS Search for Massive Binaries in the Ionizing Cluster of 30 Dor | journal=Astronomical Journal | volume=137 |issue=2 | pages=3437–3441 | date=2009 | bibcode=2009AJ....137.3437B | doi=10.1088/0004-6256/137/2/3437|arxiv = 0811.4748 }} 4. ^{{cite journal|doi=10.1051/0004-6361/201322696|title=The Wolf-Rayet stars in the Large Magellanic Cloud|journal=Astronomy & Astrophysics|volume=565|pages=A27|year=2014|last1=Hainich|first1=R.|last2=Rühling|first2=U.|last3=Todt|first3=H.|last4=Oskinova|first4=L. M.|last5=Liermann|first5=A.|last6=Gräfener|first6=G.|last7=Foellmi|first7=C.|last8=Schnurr|first8=O.|last9=Hamann|first9=W.-R.|bibcode=2014A&A...565A..27H|arxiv = 1401.5474 }} External links
6 : NGC objects|Tarantula Nebula|Dorado (constellation)|Open clusters|Large Magellanic Cloud|Star-forming regions |
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