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A three-dimensional map of the Milky Way using classical Cepheid variable stars
The Milky Way is a barred spiral galaxy, with physical properties inferred from various tracers informed by the extrapolation of structures seen in other galaxies. However, the distances of these tracers are measured indirectly and are model-dependent. We constructed a map of the Milky Way in three...
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Published in: | Science (American Association for the Advancement of Science) 2019-08, Vol.365 (6452), p.478-482 |
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creator | Skowron, Dorota M Skowron, Jan Mróz, Przemek Udalski, Andrzej Pietrukowicz, Paweł Soszyński, Igor Szymański, Michał K Poleski, Radosław Kozłowski, Szymon Ulaczyk, Krzysztof Rybicki, Krzysztof Iwanek, Patryk |
description | The Milky Way is a barred spiral galaxy, with physical properties inferred from various tracers informed by the extrapolation of structures seen in other galaxies. However, the distances of these tracers are measured indirectly and are model-dependent. We constructed a map of the Milky Way in three dimensions, based on the positions and distances of thousands of classical Cepheid variable stars. This map shows the structure of our Galaxy's young stellar population and allows us to constrain the warped shape of the Milky Way's disk. A simple model of star formation in the spiral arms reproduces the observed distribution of Cepheids. |
doi_str_mv | 10.1126/science.aau3181 |
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However, the distances of these tracers are measured indirectly and are model-dependent. We constructed a map of the Milky Way in three dimensions, based on the positions and distances of thousands of classical Cepheid variable stars. This map shows the structure of our Galaxy's young stellar population and allows us to constrain the warped shape of the Milky Way's disk. A simple model of star formation in the spiral arms reproduces the observed distribution of Cepheids.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.aau3181</identifier><identifier>PMID: 31371611</identifier><language>eng</language><publisher>United States: The American Association for the Advancement of Science</publisher><subject>Cepheid variables ; Construction ; Galactic structure ; Galaxies ; Galaxy distribution ; Milky Way ; Periodic variations ; Physical properties ; Spiral galaxies ; Star & galaxy formation ; Star formation ; Stars ; Stars & galaxies ; Stellar age ; Stellar populations ; Three dimensional models ; Tracers ; Variable stars</subject><ispartof>Science (American Association for the Advancement of Science), 2019-08, Vol.365 (6452), p.478-482</ispartof><rights>Copyright © 2019 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.</rights><rights>Copyright © 2019 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c432t-909474e561d9a2452af8cddde8b2b0c6e6ed772dcbd5a04869a8a15f928833013</citedby><cites>FETCH-LOGICAL-c432t-909474e561d9a2452af8cddde8b2b0c6e6ed772dcbd5a04869a8a15f928833013</cites><orcidid>0000-0001-9439-604X ; 0000-0002-7777-0842 ; 0000-0002-2339-5899 ; 0000-0002-0548-8995 ; 0000-0001-6364-408X ; 0000-0002-6212-7221 ; 0000-0001-5207-5619 ; 0000-0003-4084-880X ; 0000-0002-9245-6368 ; 0000-0002-9326-9329 ; 0000-0001-7016-1692 ; 0000-0002-2335-1730</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,2884,2885,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/31371611$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Skowron, Dorota M</creatorcontrib><creatorcontrib>Skowron, Jan</creatorcontrib><creatorcontrib>Mróz, Przemek</creatorcontrib><creatorcontrib>Udalski, Andrzej</creatorcontrib><creatorcontrib>Pietrukowicz, Paweł</creatorcontrib><creatorcontrib>Soszyński, Igor</creatorcontrib><creatorcontrib>Szymański, Michał K</creatorcontrib><creatorcontrib>Poleski, Radosław</creatorcontrib><creatorcontrib>Kozłowski, Szymon</creatorcontrib><creatorcontrib>Ulaczyk, Krzysztof</creatorcontrib><creatorcontrib>Rybicki, Krzysztof</creatorcontrib><creatorcontrib>Iwanek, Patryk</creatorcontrib><title>A three-dimensional map of the Milky Way using classical Cepheid variable stars</title><title>Science (American Association for the Advancement of Science)</title><addtitle>Science</addtitle><description>The Milky Way is a barred spiral galaxy, with physical properties inferred from various tracers informed by the extrapolation of structures seen in other galaxies. However, the distances of these tracers are measured indirectly and are model-dependent. We constructed a map of the Milky Way in three dimensions, based on the positions and distances of thousands of classical Cepheid variable stars. This map shows the structure of our Galaxy's young stellar population and allows us to constrain the warped shape of the Milky Way's disk. A simple model of star formation in the spiral arms reproduces the observed distribution of Cepheids.</description><subject>Cepheid variables</subject><subject>Construction</subject><subject>Galactic structure</subject><subject>Galaxies</subject><subject>Galaxy distribution</subject><subject>Milky Way</subject><subject>Periodic variations</subject><subject>Physical properties</subject><subject>Spiral galaxies</subject><subject>Star & galaxy formation</subject><subject>Star formation</subject><subject>Stars</subject><subject>Stars & galaxies</subject><subject>Stellar age</subject><subject>Stellar populations</subject><subject>Three dimensional models</subject><subject>Tracers</subject><subject>Variable 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subjects | Cepheid variables Construction Galactic structure Galaxies Galaxy distribution Milky Way Periodic variations Physical properties Spiral galaxies Star & galaxy formation Star formation Stars Stars & galaxies Stellar age Stellar populations Three dimensional models Tracers Variable stars |
title | A three-dimensional map of the Milky Way using classical Cepheid variable stars |
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