Price-Whelan 1
http://dbpedia.org/resource/Price-Whelan_1
Price-Whelan 1 (en abrégé PW 1) est une association stellaire dont la découverte a été annoncée en novembre 2018 par et ses collaborateurs.
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Price-Whelan 1 (PW 1) is a young stellar association or disrupting star cluster with low metallicity and extragalactic origin, more specifically the leading arm of the Magellanic gas stream originating in the Magellanic Clouds. Price-Whelan 1 was discovered by Adrian Price-Whelan using Gaia data and additional cluster members were identified using DECam data. The star cluster contains less than a thousand stars. The existence of Price-Whelan 1 suggests that the stream of gas extending from the Magellanic Clouds to our Milky Way is about half as far from the Milky Way as previously thought.
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Price-Whelan 1
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Price-Whelan 1
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Price-Whelan 1
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Open cluster
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Price-Whelan 1 (en abrégé PW 1) est une association stellaire dont la découverte a été annoncée en novembre 2018 par et ses collaborateurs.
rdf:langString
Price-Whelan 1 (PW 1) is a young stellar association or disrupting star cluster with low metallicity and extragalactic origin, more specifically the leading arm of the Magellanic gas stream originating in the Magellanic Clouds. Price-Whelan 1 was discovered by Adrian Price-Whelan using Gaia data and additional cluster members were identified using DECam data. The star cluster contains less than a thousand stars. The existence of Price-Whelan 1 suggests that the stream of gas extending from the Magellanic Clouds to our Milky Way is about half as far from the Milky Way as previously thought.
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