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<article article-type="research-article" dtd-version="1.3" 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" xml:lang="ru"><front><journal-meta><journal-id journal-id-type="publisher-id">kaz29</journal-id><journal-title-group><journal-title xml:lang="ru">Вестник Казахстанско-Британского технического университета</journal-title><trans-title-group xml:lang="en"><trans-title>Herald of the Kazakh-British Technical University</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">1998-6688</issn><issn pub-type="epub">2959-8109</issn><publisher><publisher-name>Казахстанско-Британский Технический Университет</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.55452/1998-6688-2025-22-4-279-294</article-id><article-id custom-type="elpub" pub-id-type="custom">kaz29-2300</article-id><article-categories><subj-group subj-group-type="heading"><subject>Research Article</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="ru"><subject>МАТЕМАТИЧЕСКИЕ НАУКИ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>MATHEMATICAL SCIENCES</subject></subj-group></article-categories><title-group><article-title>О НЕКОТОРЫХ ПОДКЛАССАХ КЛАССОВ ПОЧТИ ВЫПУКЛЫХ  И ДВАЖДЫ ПОЧТИ ВЫПУКЛЫХ ФУНКЦИЙ</article-title><trans-title-group xml:lang="en"><trans-title>ABOUT SOME SUBCLASSES OF CLASSES OF CLOSE-TO-CONVEX  AND DOUBLY CLOSE-TO-CONVEX FUNCTIONS</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-2278-2723</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Майер</surname><given-names>Ф. Ф.</given-names></name><name name-style="western" xml:lang="en"><surname>Maiyer</surname><given-names>F. F.</given-names></name></name-alternatives><bio xml:lang="ru"><p>канд. физ.-матем. наук, профессор</p><p>г. Костанай</p></bio><bio xml:lang="en"><p>Cand. Phys.-Math. Sc., Professor</p><p>Kostanay</p></bio><email xlink:type="simple">maiyer@mail.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0003-1926-8958</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Тастанов</surname><given-names>М. Г.</given-names></name><name name-style="western" xml:lang="en"><surname>Tastanov</surname><given-names>M. G.</given-names></name></name-alternatives><bio xml:lang="ru"><p>канд. физ.-матем. наук, профессор</p><p>г. Костанай</p></bio><bio xml:lang="en"><p>Cand. Phys.-Math. Sc., Professor</p><p>Kostanay</p></bio><email xlink:type="simple">tastao@mail.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0001-5143-0260</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Утемисова</surname><given-names>А. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Utemissova</surname><given-names>A. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>канд. пед. наук, ассоциированный профессор</p><p>г. Костанай</p></bio><bio xml:lang="en"><p>Cand. Ped. Sc., Associate Professor</p><p>Kostanay</p></bio><email xlink:type="simple">anar_utemisova@mail.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0009-0003-6007-0254</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Калаков</surname><given-names>Б. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Kalakov</surname><given-names>B. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>канд. физ.-матем. наук</p><p>г. Костанай</p></bio><bio xml:lang="en"><p>Cand. Phys.-Math. Sc.</p><p>Kostanay</p></bio><email xlink:type="simple">kalakov1968@gmail.com</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru">Костанайский региональный университет им. Ахмета Байтұрсынұлы<country>Казахстан</country></aff><aff xml:lang="en">Akhmet Baitursynuly Kostanay Regional University<country>Kazakhstan</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2025</year></pub-date><pub-date pub-type="epub"><day>23</day><month>12</month><year>2025</year></pub-date><volume>22</volume><issue>4</issue><fpage>279</fpage><lpage>294</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Майер Ф.Ф., Тастанов М.Г., Утемисова А.А., Калаков Б.А., 2025</copyright-statement><copyright-year>2025</copyright-year><copyright-holder xml:lang="ru">Майер Ф.Ф., Тастанов М.Г., Утемисова А.А., Калаков Б.А.</copyright-holder><copyright-holder xml:lang="en">Maiyer F.F., Tastanov M.G., Utemissova A.A., Kalakov B.A.</copyright-holder><license xml:lang="ru" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>Данная работа распространяется под лицензией Creative Commons Attribution 4.0.</license-p></license><license xml:lang="en" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>This work is licensed under a Creative Commons Attribution 4.0 License.</license-p></license></permissions><self-uri xlink:href="https://vestnik.kbtu.edu.kz/jour/article/view/2300">https://vestnik.kbtu.edu.kz/jour/article/view/2300</self-uri><abstract><p>Известно, что класс  почти выпуклых функций задается условием положительности функционала  со звездообразной функцией . Замена звездообразной функции  на выпуклую приводит к известному подклассу  класса . В настоящей статье вводится обобщение класса  на случай, когда множество значений  содержится в области специального вида, которая в частном случае может совпадать и с полуплоскостью. Также обобщение связано с расширением класса  до определенного подкласса класса нормированных дважды почти выпуклых функций. Многообразие частных случаев области специального вида и переход к дважды почти выпуклым функциям позволяет получить как новые оригинальные результаты, так и обобщения ранее известных результатов. Основные исследования данной статьи направлены на доказательство теорем об искажении, нахождение радиусов выпуклости рассматриваемых классов функций и обоснование точности полученных результатов. Также установлена связь введенного класса функций с некоторым новым классом дважды почти звездообразных функций. Для данного класса и его подклассов также получены новые результаты в виде теорем о росте и радиусе звездообразности и обобщения ранее известных результатов.</p></abstract><trans-abstract xml:lang="en"><p>It is known that the class  close-to-convex functions is defined by the condition of positivity of the functional  with a starlike function . Replacing the starlike function  with a convex one leads to a known subclass  of the class . In this article, we introduce a generalization of the class  to the case when the set of values  is contained in a region of a special type, which, in a particular case, can coincide with a half-plane. The generalization is also associated with the extension of the class  to a certain subclass of the class of normalized doubly close-to-convex functions. The diversity of special cases of a domain of a special type and the transition to doubly close-to-convex functions allows us to obtain both new original results and generalizations of previously known results. The main research of this article is aimed at proving theorems on distortion, finding the radii of convexity of the considered classes of functions and justifying the accuracy of the obtained results. A connection has also been established between the introduced class of functions and a certain new class of doubly close-to-starlike functions, special cases of which have been actively studied in recent years. For this class and its subclasses, new results have also been obtained in the form of theorems on growth and radius of starlikeness and generalization of previously known results.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>звездообразные функции</kwd><kwd>почти звездообразные функции</kwd><kwd>почти выпуклые функции</kwd><kwd>теоремы искажения</kwd><kwd>радиусы выпуклости</kwd><kwd>теоремы роста</kwd><kwd>радиусы звездообразности</kwd></kwd-group><kwd-group xml:lang="en"><kwd>starlike functions</kwd><kwd>close-to-starlike functions</kwd><kwd>close-to-convex functions</kwd><kwd>distortion theorems</kwd><kwd>radii of convexity</kwd><kwd>growth theorems</kwd><kwd>radii of starlikeness</kwd></kwd-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Kaplan W. Close-to-convex schlicht functions // Michigan Math. 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