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<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:ali="http://www.niso.org/schemas/ali/1.0/" article-type="research-article" dtd-version="1.2" xml:lang="en"><front><journal-meta><journal-id journal-id-type="publisher-id">Astronomy Reports</journal-id><journal-title-group><journal-title xml:lang="en">Astronomy Reports</journal-title><trans-title-group xml:lang="ru"><trans-title>Астрономический журнал</trans-title></trans-title-group></journal-title-group><issn publication-format="print">0004-6299</issn><issn publication-format="electronic">3034-5170</issn><publisher><publisher-name xml:lang="en">The Russian Academy of Sciences</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">355482</article-id><article-id pub-id-type="doi">10.7868/S3034518925110028</article-id><article-categories><subj-group subj-group-type="toc-heading" xml:lang="en"><subject>Articles</subject></subj-group><subj-group subj-group-type="toc-heading" xml:lang="ru"><subject>СТАТЬИ</subject></subj-group><subj-group subj-group-type="article-type"><subject>Research Article</subject></subj-group></article-categories><title-group><article-title xml:lang="en">THE PLACE OF THE RADCLIFFE WAVE IN THE LOCAL SYSTEM</article-title><trans-title-group xml:lang="ru"><trans-title>МЕСТО ВОЛНЫ РЭДКЛИФФА В МЕСТНОЙ СИСТЕМЕ</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Bobylev</surname><given-names>V. V</given-names></name><name xml:lang="ru"><surname>Бобылев</surname><given-names>В. В</given-names></name></name-alternatives><email>bob-v-vzz@rambler.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Ikhsanov</surname><given-names>N. R</given-names></name><name xml:lang="ru"><surname>Ихсанов</surname><given-names>Н. Р</given-names></name></name-alternatives><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Bajkova</surname><given-names>A. T</given-names></name><name xml:lang="ru"><surname>Байкова</surname><given-names>А. Т</given-names></name></name-alternatives><xref ref-type="aff" rid="aff1"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">Central Astronomical Observatory of the Russian Academy of Sciences, Pulkovo</institution></aff><aff><institution xml:lang="ru">Главная (Пулковская) астрономическая обсерватория РАН</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2025-11-15" publication-format="electronic"><day>15</day><month>11</month><year>2025</year></pub-date><volume>102</volume><issue>11</issue><issue-title xml:lang="en">VOL 102, NO11 (2025)</issue-title><issue-title xml:lang="ru">ТОМ 102, №11 (2025)</issue-title><fpage>975</fpage><lpage>988</lpage><history><date date-type="received" iso-8601-date="2025-12-02"><day>02</day><month>12</month><year>2025</year></date></history><permissions><copyright-statement xml:lang="en">Copyright ©; 2025, Russian Academy of Sciences</copyright-statement><copyright-statement xml:lang="ru">Copyright ©; 2025, Российская академия наук</copyright-statement><copyright-year>2025</copyright-year><copyright-holder xml:lang="en">Russian Academy of Sciences</copyright-holder><copyright-holder xml:lang="ru">Российская академия наук</copyright-holder><ali:free_to_read xmlns:ali="http://www.niso.org/schemas/ali/1.0/" start_date="2026-11-15"/></permissions><self-uri xlink:href="https://journals.rcsi.science/0004-6299/article/view/355482">https://journals.rcsi.science/0004-6299/article/view/355482</self-uri><abstract xml:lang="en"><p>A review of publications devoted to the study of the characteristics of the Radcliffe wave is given. The advent of mass measurements of radial velocities of stars has recently led to a number of interesting results obtained from the analysis of spatial velocities of stars and open star clusters. An important place in the work is given to issues related to the clarification of the direct or indirect influence of magnetic fields on the process of formation of the Radcliffe wave. The hypothesis of Parker instability of the galactic magnetic field as one of the reasons for the formation of wave-type inhomogeneities in the galactic disk is discussed.</p></abstract><trans-abstract xml:lang="ru"><p>Дан обзор публикаций, посвященных изучению характеристик волны Рэдклиффа. Появление массовых измерений лучевых скоростей звезд привело в последнее время к получению ряда интересных результатов, найденных из анализа пространственных скоростей молодых звезд и рассеянных звездных скоплений. Важное место в работе уделено вопросам, связанным с выяснением прямого или косвенного влияния магнитных полей на процесс формирования волны Рэдклиффа. Обсуждается гипотеза о Паркеровской неустойчивости галактического магнитного поля как одной из причин формирования неоднородностей волнообразного типа в галактическом диске.</p></trans-abstract><kwd-group xml:lang="en"><kwd>Local star system</kwd><kwd>Orion arm</kwd><kwd>Gould Belt</kwd><kwd>Radcliffe wave</kwd><kwd>young stars</kwd></kwd-group><kwd-group xml:lang="ru"><kwd>Местная система звезд</kwd><kwd>рукав Ориона</kwd><kwd>Пояс Гулда</kwd><kwd>волна Рэдклиффа</kwd><kwd>молодые звезды</kwd></kwd-group></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>H. Mineur, Monthly Not. Roy. Astron. Soc. 90, 789 (1930).</mixed-citation></ref><ref id="B2"><label>2.</label><mixed-citation>К. Ф. 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