'The Spatial Structure of Young Stellar Clusters. Moore, Cambridge University Press, ISBN 6-5 (2002) ^ 'Cambridge Deep Sky Companions - The Caldwell Objects', S.J.'A Parsec-Scale Outflow in the Rosette Molecular Cloud?'. Centre de donnГ©es astronomiques de Strasbourg. Oklahoma Governor Kevin Stitt signed it into law April 22, 2019. On Apthe Oklahoma Legislature passed HB1292 making the Rosette Nebula as the official state astronomical object. This is significantly hotter than the 10,000 K plasmas seen in HII regions, and is likely attributed to the shock-heated winds from the massive O-type stars. ДЄ diffuse X-ray glow is also seen between the stars in the bubble, which has been attributed to a super-hot plasma with temperatures ranging from 1 to 10 million K. Most of the ongoing star-formation activity is occurring in the dense molecular cloud to the south east of the bubble. Altogether, approximately 2500 young stars lie in this star-forming complex, including the massive O-type stars HD 46223 and HD 46150, which are primarily responsible for blowing the ionized bubble. The mass of the nebula is estimated to be around 10,000 solar masses.ДЄ survey of the nebula with the Chandra X-ray Observatory has revealed the presence of numerous new-born stars inside optical Rosette Nebula and studded within a dense molecular cloud. The radiation from the young stars excites the atoms in the nebula, causing them to emit radiation themselves producing the emission nebula we see. The cluster and nebula lie at a distance of 5,000 light-years from Earth and measure roughly 130 light years in diameter. NGC 2244 вЂ“ The open cluster within the nebula (Discovered by John Flamsteed in 1690).

NGC 2239 вЂ“ Part of the nebulous region (Discovered by John Herschel).NGC 2237 вЂ“ Part of the nebulous region (Also used to denote whole nebula).The complex has the following New General Catalogue (NGC) designations: The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the stars of the cluster having been formed from the nebula's matter. The Rosette Nebula (also known as Caldwell 49) is an H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. Telescope: Takahashi TOA 130 Postprocessing with PixInsight

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