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One of the most massive stars in the Galaxy may have formed in isolation

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Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521, , , , , , , , , and 1248 other author(s). (2020)cite arxiv:2009.01190Comment: 39 pages, 13 figures; data available at https://dcc.ligo.org/P2000158-v4/public.GW190521: A Binary Black Hole Merger with a Total Mass of $150 ~ M_ødot$, , , , , , , , , and 1247 other author(s). (2020)cite arxiv:2009.01075Comment: Supplementary Material at https://dcc.ligo.org/LIGO-P2000020/Public.A gravitational-wave standard siren measurement of the Hubble constant, , , , , , , , , and 1304 other author(s). (2017)cite arxiv:1710.05835Comment: 26 pages, 5 figures, Nature in press. For more information see https://dcc.ligo.org/LIGO-P1700296/public.The Physics of the B Factories, , , , , , , , , and 2024 other author(s). The European Physical Journal C, (Jul 8, 2014)Physics Performance Report for PANDA: Strong Interaction Studies with Antiprotons, , , , , , , , , and 406 other author(s). (Mar 23, 2009)One of the most massive stars in the Galaxy may have formed in isolation, , , , , and . (2013)cite arxiv:1309.7651Comment: 10 pages, 10 figures, MNRAS, in press.Searches for continuous gravitational waves from nine young supernova remnants, , , , , , , , , and 886 other author(s). (Dec 18, 2014)Observation of Gravitational Waves from a Binary Black Hole Merger, , , , , , , , , and 1001 other author(s). Phys. Rev. Lett., (February 2016)Diffuse Reflectance of Whole Blood: Model for a Diverging Light Beam., and . IEEE Trans. Biomed. Eng., 34 (10): 826-834 (1987)