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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">647660</article-id><article-id pub-id-type="doi">10.31857/S0004629924100023</article-id><article-id pub-id-type="edn">JMDAJJ</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">Destruction of open star clusters and the radius-mass relationship</article-title><trans-title-group xml:lang="ru"><trans-title>Распад рассеянных звездных скоплений и соотношение радиус-масса</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Tutukov</surname><given-names>A. V.</given-names></name><name xml:lang="ru"><surname>Тутуков</surname><given-names>А. В.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>svvs@ya.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Vereshchagin</surname><given-names>S. V.</given-names></name><name xml:lang="ru"><surname>Верещагин</surname><given-names>С. В.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>svvs@ya.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Chupina</surname><given-names>N. V.</given-names></name><name xml:lang="ru"><surname>Чупина</surname><given-names>Н. В.</given-names></name></name-alternatives><address><country country="RU">Russian Federation</country></address><email>svvs@ya.ru</email><xref ref-type="aff" rid="aff1"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">Institute of Astronomy, Russian Academy of Sciences</institution></aff><aff><institution xml:lang="ru">Институт астрономии РАН</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2024-10-15" publication-format="electronic"><day>15</day><month>10</month><year>2024</year></pub-date><volume>101</volume><issue>10</issue><fpage>885</fpage><lpage>902</lpage><history><date date-type="received" iso-8601-date="2025-01-28"><day>28</day><month>01</month><year>2025</year></date></history><permissions><copyright-statement xml:lang="en">Copyright ©; 2024, The Russian Academy of Sciences</copyright-statement><copyright-statement xml:lang="ru">Copyright ©; 2024, Российская академия наук</copyright-statement><copyright-year>2024</copyright-year><copyright-holder xml:lang="en">The Russian Academy of Sciences</copyright-holder><copyright-holder xml:lang="ru">Российская академия наук</copyright-holder></permissions><self-uri xlink:href="https://journals.eco-vector.com/0004-6299/article/view/647660">https://journals.eco-vector.com/0004-6299/article/view/647660</self-uri><abstract xml:lang="en"><p>The processes of formation and six mechanisms of disintegration of open star clusters (OSCs) are considered. Analytical estimates of the rates of OSC disintegration are made for the following mechanisms: loss of the initial gas component of OSCs, mass loss due to supernovae explosions and planetary nebula formation, pair interactions of OSC stars, acceleration of stars by binary systems of OSCs, interaction of OSC stars with stars of the Galactic disk, collisions of OSCs with giant molecular clouds (GMCs) at the front of a spiral wave. The destruction of OSCs is accompanied by the formation of a stellar stream. An analysis of the radius-mass ratio of the OSC core (<italic>RM</italic>) allowed us to conclude that it probably does not reflect the disintegration mechanism and is a product of observational selection effects. The evolution of an individual OSC in the <italic>R-M</italic> plane is determined by the initial density and external conditions.</p></abstract><trans-abstract xml:lang="ru"><p>Рассмотрены процессы образования и шесть механизмов распада рассеянных звездных скоплений (РЗС). Выполнены аналитические оценки скоростей распада РЗСв результате действия следующих механизмов: потеря начального газового компонента РЗС, потеря вещества из-за вспышек сверхновых звезд и образования планетарных туманностей, парные взаимодействия звезд РЗС, ускорение звезд двойными системами РЗС, взаимодействие звезд РЗС со звездами диска Галактики, столкновение РЗС с гигантскими молекулярными облаками (ГМО) на фронте спиральной волны. Разрушение РЗС сопровождается образованием звездного потока. Анализ соотношения радиус-масса ядра РЗС (<italic>RM</italic>) позволил сделать вывод о том, что оно, вероятно, не связано с механизмом распада и является продуктом эффектов наблюдательной селекции. Эволюция индивидуального РЗС в плоскости <italic>R</italic><italic>–</italic><italic>M</italic> определяется начальной плотностью и внешними условиями.</p></trans-abstract><kwd-group xml:lang="en"><kwd>open star clusters</kwd><kwd>cluster evolution</kwd></kwd-group><kwd-group xml:lang="ru"><kwd>рассеянные звездные скопления</kwd><kwd>эволюция скоплений</kwd></kwd-group><funding-group/></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>H. Shapley, John G. Wolbach Library, Harvard-Smithsonian Center for Astrophysics (HarMo) 2 (1930).</mixed-citation></ref><ref id="B2"><label>2.</label><mixed-citation>B. Hertzsprung, Bulletin of the Astronomical Institutes of the Netherlands 1, 218 (1923).</mixed-citation></ref><ref id="B3"><label>3.</label><mixed-citation>R. Trumpler, Lick Observatory bulletin 14, 154 (1930).</mixed-citation></ref><ref id="B4"><label>4.</label><mixed-citation>O.J. Eggen, A.R. Sandage, Monthly Not. Roy. Astron. Soc. 119, 255 (1959).</mixed-citation></ref><ref id="B5"><label>5.</label><mixed-citation>Ch. Messier, Connoissance des Temps ou des Mouvements Célestes for 1784, 227 (1781).</mixed-citation></ref><ref id="B6"><label>6.</label><mixed-citation>W. Herschel, Philosoph. Trans. Roy. Soc. of London 76, 457 (1786).</mixed-citation></ref><ref id="B7"><label>7.</label><mixed-citation>R. Proctor, Monthly Not. Roy. Astron. Soc. 30, 50 (1869).</mixed-citation></ref><ref id="B8"><label>8.</label><mixed-citation>A. Eddington, Nature 106, 14 (1920).</mixed-citation></ref><ref id="B9"><label>9.</label><mixed-citation>S. Chandrasekhar, Astrophys J. 67, 206 (1938).</mixed-citation></ref><ref id="B10"><label>10.</label><mixed-citation>H. Jonson, A. Sandage, Astrophys. J. 121, 616 (1955).</mixed-citation></ref><ref id="B11"><label>11.</label><mixed-citation>I. King, Astron. J. 63, 265 (1958).</mixed-citation></ref><ref id="B12"><label>12.</label><mixed-citation>O. Eggen, G. Herbig, Monthly Not. Roy. Astron. Soc. 137, 111 (1967).</mixed-citation></ref><ref id="B13"><label>13.</label><mixed-citation>R. Larson, Monthly Not. Roy. Astron. Soc. 147, 323 (1970).</mixed-citation></ref><ref id="B14"><label>14.</label><mixed-citation>S. Aarseth, Astron. and Ск 35, 237 (1974).</mixed-citation></ref><ref id="B15"><label>15.</label><mixed-citation>A. Tutukov, Astron. and Astrophys. 70, 57 (1978).</mixed-citation></ref><ref id="B16"><label>16.</label><mixed-citation>D.A. Vandenberg, Astrophys. J. Suppl. Ser. 51, 29 (1983).</mixed-citation></ref><ref id="B17"><label>17.</label><mixed-citation>Ch. J. Lada, E.A. Lada, ASP Conf. Ser. 13, 3 (1991).</mixed-citation></ref><ref id="B18"><label>18.</label><mixed-citation>P. Zwart, F. Simon, P. Hut et al., Astron. and Astrophys. 337, 363 (1998).</mixed-citation></ref><ref id="B19"><label>19.</label><mixed-citation>N. Bastian, M. Gieles, ASPC 386, 353 (2008).</mixed-citation></ref><ref id="B20"><label>20.</label><mixed-citation>A. Kamlah, R. Spurzem, P. Berczik et al., Monthly Not. Roy. Astron. Soc. 516, 3266 (2022).</mixed-citation></ref><ref id="B21"><label>21.</label><mixed-citation>J.E. Wall et al., Astrophys. J. 904, 192 (2020).</mixed-citation></ref><ref id="B22"><label>22.</label><mixed-citation>A. Just, A.E. Piskunov, J.H. Klos et al., Astron. and Astrophys. 672, id. A187 (2023).</mixed-citation></ref><ref id="B23"><label>23.</label><mixed-citation>Е.L. Hunt, S. Reffert, Astron. and Astrophys. 673, A 114 (2023).</mixed-citation></ref><ref id="B24"><label>24.</label><mixed-citation>R. Larson, Monthly Not. Roy. Astron. Soc. 194, 809 (1981).</mixed-citation></ref><ref id="B25"><label>25.</label><mixed-citation>S. Pfalzner, H. Kirk, A. Sills et al., Astron. and Astrophys. 586, 68 (2016).</mixed-citation></ref><ref id="B26"><label>26.</label><mixed-citation>J. Chieze, Astron. and Astrophys. 171, 225 (1987).</mixed-citation></ref><ref id="B27"><label>27.</label><mixed-citation>A. Mok, R. Chandar, S. M. Fall, Astrophys. J. 911, 8 (2021).</mixed-citation></ref><ref id="B28"><label>28.</label><mixed-citation>S. Smith, W. Cherny, Ch. Hayes et al., Astrophys. J. 961, 92 (2024).</mixed-citation></ref><ref id="B29"><label>29.</label><mixed-citation>A. Tutukov, Astron. Rep. 63, 19 (2019).</mixed-citation></ref><ref id="B30"><label>30.</label><mixed-citation>M. Krumholz, Sh. McKee, J. Bland-Hawthorn, Ann. Rev. of Astron. and Astrophys. 57, 227 (2019).</mixed-citation></ref><ref id="B31"><label>31.</label><mixed-citation>B. Chen, G. Li, H. Yuan et al., Monthly Not. Roy. Astron. Soc. 493, 351 (2020).</mixed-citation></ref><ref id="B32"><label>32.</label><mixed-citation>N. Choksi, J.M.D. Kruijssen, Monthly Not. Roy. Astron. Soc. 507, 5492 (2021)</mixed-citation></ref><ref id="B33"><label>33.</label><mixed-citation>Y. Xing, K. Qiu, Res. in Astron. and Astrophys. 22, id.075006 (2022).</mixed-citation></ref><ref id="B34"><label>34.</label><mixed-citation>K. Neralwar, D. Colombo, A. Duarte-Cabral et al., Astron. and Astrophys. 884, 84 (2022).</mixed-citation></ref><ref id="B35"><label>35.</label><mixed-citation>J.P. Farias, S.S.R. Offner, M.Y. Grudić et al., Monthly Not. Roy. Astron. Soc. 527, 6732 (2024).</mixed-citation></ref><ref id="B36"><label>36.</label><mixed-citation>J. Yuan, Y. Wu, S. Ellingsen et al., Astrophys. J. Suppl. Ser. 231, 11 (2017).</mixed-citation></ref><ref id="B37"><label>37.</label><mixed-citation>F. Maeda, K. Ohta, Y. Fujimoto et al. Monthly Not. Roy. Astron. Soc. 493, 5045 (2020).</mixed-citation></ref><ref id="B38"><label>38.</label><mixed-citation>A. Just, S. Jacobi, B. Deis, Astron. and Astrophys. 289, 237 (2024).</mixed-citation></ref><ref id="B39"><label>39.</label><mixed-citation>M. Fujii, P. Zwart, Monthly Not. Roy. Astron. Soc. 449, 126 (2015).</mixed-citation></ref><ref id="B40"><label>40.</label><mixed-citation>M. Messa, A. Adamo, D. Calzetti et al., Monthly Not. Roy. Astron. Soc. 477, 1683 (2018).</mixed-citation></ref><ref id="B41"><label>41.</label><mixed-citation>A. Mok, R. Chandar, S.M. Fall, Astrophys. J. 893, 135 (2020).</mixed-citation></ref><ref id="B42"><label>42.</label><mixed-citation>M. Kobayashi, S.I. Inutsuka, H. Kobayashi, Astrophys. J. 836, 175 (2017).</mixed-citation></ref><ref id="B43"><label>43.</label><mixed-citation>A. Tutukov, B. Shustov, Astrophysics 63, 552 (2020).</mixed-citation></ref><ref id="B44"><label>44.</label><mixed-citation>P. Kroupa, IAUS 241, 109 (2007).</mixed-citation></ref><ref id="B45"><label>45.</label><mixed-citation>А. Масевич, А. Тутуков. Эволюция звезд: теория и наблюдения (М: Наука, 1988).</mixed-citation></ref><ref id="B46"><label>46.</label><mixed-citation>B.M. Shustov, A.V. Tutukov, Astron. Rep. 62, 784 (2018).</mixed-citation></ref><ref id="B47"><label>47.</label><mixed-citation>H. Lamers, H. Baumgardt, M. Gieles, Monthly Not. Roy. Astron. Soc. 433, 1378 (2013).</mixed-citation></ref><ref id="B48"><label>48.</label><mixed-citation>E. Vesperini, J. Hogg, J. Webb et al., Monthly Not. Roy. Astron. Soc. 476, 2731 (2018).</mixed-citation></ref><ref id="B49"><label>49.</label><mixed-citation>K. Wang, E. Peng, Ch. Liu et al., Nature 623, 296 (2023).</mixed-citation></ref><ref id="B50"><label>50.</label><mixed-citation>M. Kissler-Patig, A. Jordan, N. Bastian, Astron. and Astrophys. 448, 1031 (2006).</mixed-citation></ref><ref id="B51"><label>51.</label><mixed-citation>Ch-Ch He, M. Ricotti, S. Geen, Monthly Not. Roy. Astron. Soc. 489, 1880 (2019).</mixed-citation></ref><ref id="B52"><label>52.</label><mixed-citation>H. Li, O. Gnedin, N. Gnedin, Astrophys. J. 861, id. 107 (2018).</mixed-citation></ref><ref id="B53"><label>53.</label><mixed-citation>M. Grudic, P. Horkins, E. Lee et al., Monthly Not. Roy. Astron. Soc. 488, 1501 (2019).</mixed-citation></ref><ref id="B54"><label>54.</label><mixed-citation>E. Diaz-Marquez, R. Grau, G. Busquet et al., Astron. and Astrophys. 682, A180 (2024).</mixed-citation></ref><ref id="B55"><label>55.</label><mixed-citation>S. Ray, S. Dhiwar, J. Bagehi et al., Monthly Not. Roy. Astron. Soc. 527, 9999 (2024).</mixed-citation></ref><ref id="B56"><label>56.</label><mixed-citation>Z. He, K. Wang, Y. Luo et al., Astrophys J. Suppl. Ser. 262, 7 (2022).</mixed-citation></ref><ref id="B57"><label>57.</label><mixed-citation>Ya. O. Chumak, A.S. Rastorguev, Astronomy Letters 32, 157 (2006).</mixed-citation></ref><ref id="B58"><label>58.</label><mixed-citation>S. Meingast, J. Alves, Astron. and Astrophys. 621, L3 (2019).</mixed-citation></ref><ref id="B59"><label>59.</label><mixed-citation>S. Röser, E. Schilbach, B. Goldman, Astron. and Astrophys. 621, L2 (2019).</mixed-citation></ref><ref id="B60"><label>60.</label><mixed-citation>S. Linden, A. Evans, L. Amus et al., Astrophys. J. 944, 55 (2023).</mixed-citation></ref><ref id="B61"><label>61.</label><mixed-citation>O. Gunes, Y. Karatas, Ch. Bonatto, Astron. Nachrichten. 338, 464 (2017).</mixed-citation></ref><ref id="B62"><label>62.</label><mixed-citation>К. Маршал. Задача трех тел (М: Наука, 2005).</mixed-citation></ref><ref id="B63"><label>63.</label><mixed-citation>A. Tutukov, M. Sizova, S. Vereshchagin, Astron. Rep. 64, 827 (2020).</mixed-citation></ref><ref id="B64"><label>64.</label><mixed-citation>E. Vaher, D. Hobbs, P. McMillan et al., Astron. and Astrophys. 679, A105 (2023).</mixed-citation></ref><ref id="B65"><label>65.</label><mixed-citation>Y. Hirata, T. Mirase, J. Nishi et al., Publ. Astron. Soc. Jap. 76, 65 (2024).</mixed-citation></ref><ref id="B66"><label>66.</label><mixed-citation>N.V. Kharchenko et al., J/A+A/558/A53/catalog (2013).</mixed-citation></ref><ref id="B67"><label>67.</label><mixed-citation>S. Roser, E. Schilbach, Astron. and Astrophys. 638, 9 (2020).</mixed-citation></ref><ref id="B68"><label>68.</label><mixed-citation>G. Thomas, B. Famaey, G. Monari et al., Astron. and Astrophys. 678, 180 (2023).</mixed-citation></ref><ref id="B69"><label>69.</label><mixed-citation>S. Goodwin, N. Bastian, Monthly Not. Roy. Astron. Soc. 373, 152 (2006).</mixed-citation></ref><ref id="B70"><label>70.</label><mixed-citation>H. Lamers, M. Gieles, Astron. and Astrophys. 455, 17 (2006).</mixed-citation></ref><ref id="B71"><label>71.</label><mixed-citation>D. Cook, L. Lee, A. Adamo et al., Monthly Not. Roy. Astron. Soc. 519, 3749 (2023).</mixed-citation></ref><ref id="B72"><label>72.</label><mixed-citation>M. Krumnolz, C. McKee, Monthly Not. Roy. Astron. Soc. 494, 624 (2020).</mixed-citation></ref><ref id="B73"><label>73.</label><mixed-citation>N. Bastian, M. Gieles, H. Lamers et al., Astron. and Astrophys. 431, 905 (2005).</mixed-citation></ref><ref id="B74"><label>74.</label><mixed-citation>C. Lada, E. Lada, Ann. Rev. of Astron. and Astrophys. 41, 57 (2003).</mixed-citation></ref><ref id="B75"><label>75.</label><mixed-citation>S. Pfalzner, T. Kaczmarek, Astron. and Astrophys. 559, 38 (2013).</mixed-citation></ref><ref id="B76"><label>76.</label><mixed-citation>J. Maiz Apellzner, M. Gonzalez, R. Barba et al., Astron. and Astrophys. 657, 12 (2022).</mixed-citation></ref><ref id="B77"><label>77.</label><mixed-citation>J. Balin, Astrophys. J. 863, 99 (2018).</mixed-citation></ref><ref id="B78"><label>78.</label><mixed-citation>A. Eddington, Monthly Not. Roy. Astron. Soc. 76, 572 (1916).</mixed-citation></ref><ref id="B79"><label>79.</label><mixed-citation>В. Амбарцумян, Ученые зап. ЛГУ, Сер. мат. 4, 19 (1938).</mixed-citation></ref><ref id="B80"><label>80.</label><mixed-citation>L. Spitzer, Monthly Not. Roy. Astron. Soc. 100, 396 (1940).</mixed-citation></ref><ref id="B81"><label>81.</label><mixed-citation>S. Chandrasekhar, Astrophys. J. 98, 54 (1943).</mixed-citation></ref><ref id="B82"><label>82.</label><mixed-citation>S. Mc Millan, Astrophys. J. 307, 126 (1986).</mixed-citation></ref><ref id="B83"><label>83.</label><mixed-citation>M. Fujii, M. Iwasawa, Y. Funato et al., Astrophys. J. 686, 1082 (2008).</mixed-citation></ref><ref id="B84"><label>84.</label><mixed-citation>M. Giersz, D. Heggie, J. Hurley et al., Monthly Not. Roy. Astron. Soc. 431, 2184 (8013).</mixed-citation></ref><ref id="B85"><label>85.</label><mixed-citation>H. Lamers, M. Gieles, Astron. and Astrophys. 455, 17 (2006).</mixed-citation></ref><ref id="B86"><label>86.</label><mixed-citation>F. Anders, T. Kantat-Gaudin, I. Quadrino, Astron. and Astrophys. 645, 2 (2021).</mixed-citation></ref><ref id="B87"><label>87.</label><mixed-citation>Л.Э. Гуревич, Б.Ю. Левин, Доклады Академии наук СССР 70, 781 (1950).</mixed-citation></ref><ref id="B88"><label>88.</label><mixed-citation>A. Tutukov, N. Chupina, S. Vereshchagin, Astron. Rep. 67, 1418 (2023).</mixed-citation></ref><ref id="B89"><label>89.</label><mixed-citation>J. Kirkpatrick, F. Marocco, Ch. Geling et al., Astrophys. J. Supp. Ser. 271, id.55 (2024).</mixed-citation></ref><ref id="B90"><label>90.</label><mixed-citation>D. Horta, A. Price-Whelan, D. Hogg et al., Astrophys. J. 962, id.165 (2024).</mixed-citation></ref><ref id="B91"><label>91.</label><mixed-citation>J. Donada, F. Andres, C. Jordi et al., Astron. and Astrophys. 675, id.A89 (2023).</mixed-citation></ref><ref id="B92"><label>92.</label><mixed-citation>J. Darbinhausen, M. Marks, P. Kroupa, Monthly Not. Roy. Astron. Soc. 510, 413 (2022).</mixed-citation></ref><ref id="B93"><label>93.</label><mixed-citation>M. Wilkinson, J. Hurley, A. Mackey et al., Monthly Not. Roy. Astron. Soc. 343, 1025 (2003).</mixed-citation></ref><ref id="B94"><label>94.</label><mixed-citation>D.C. Heggie, Monthly Not. Roy. Astron. Soc. 173, 729 (1975).</mixed-citation></ref><ref id="B95"><label>95.</label><mixed-citation>J. Hills, Astron. J. 80, 809 (1975).</mixed-citation></ref><ref id="B96"><label>96.</label><mixed-citation>A. Tokovinin, Monthly Not. Roy. Astron. Soc. 389, 925 (2008).</mixed-citation></ref><ref id="B97"><label>97.</label><mixed-citation>D. Miller, I. Caiazzo, J. Heyl et al., Astrophys. J. Lett. 956, id.L41 (2023).</mixed-citation></ref><ref id="B98"><label>98.</label><mixed-citation>L. Wang, A. Tani Kawa, M. Fujii, Monthly Not. Roy. Astron. Soc. 509, 4713 (2022).</mixed-citation></ref><ref id="B99"><label>99.</label><mixed-citation>N. Dickson, P. Smith, V. Ytnault-Brunet et al., Monthly Not. Roy. Astron. Soc. 529, pp.331 (2023).</mixed-citation></ref><ref id="B100"><label>100.</label><mixed-citation>T. Van Albade, J. Gorkom, Astron. and Astrophys. 54, 121 (1977).</mixed-citation></ref><ref id="B101"><label>101.</label><mixed-citation>J.W. Lee, Astrophys. J. 961, id.227 (2024).</mixed-citation></ref><ref id="B102"><label>102.</label><mixed-citation>L. Saleh, J. Barnes, Monthly Not. Roy. Astron. Soc. 527, 8551 (2024).</mixed-citation></ref><ref id="B103"><label>103.</label><mixed-citation>S. White, Monthly Not. Roy. Astron. Soc. 189, 831 (1979).</mixed-citation></ref><ref id="B104"><label>104.</label><mixed-citation>S. Van den Berg, D. McClure, Astron. and Astrophys. 88, 360 (1980).</mixed-citation></ref><ref id="B105"><label>105.</label><mixed-citation>M. Gieles, S. Portegies Zwart, H. Baumgardt, Monthly Not. Roy. Astron. Soc. 371, 793 (2006).</mixed-citation></ref><ref id="B106"><label>106.</label><mixed-citation>P. Solomon, L. Sandos, N. Scoville, IAUS 84, 35 (1979).</mixed-citation></ref><ref id="B107"><label>107.</label><mixed-citation>Ch. Lada, T. Dame, Astrophys J. 898, 3 (2020).</mixed-citation></ref><ref id="B108"><label>108.</label><mixed-citation>T. Nony, R. Galvan-Madrid, N. Brouiller et al., Astron. and Astrophys. 687, id.A84 (2024).</mixed-citation></ref><ref id="B109"><label>109.</label><mixed-citation>B. Bhatt, A. Pandey, H. Mahra, Astrophys. and Space Sci. 129, 293 (1987).</mixed-citation></ref><ref id="B110"><label>110.</label><mixed-citation>M. Gieles, H. Baumgardt, D.C. Heggie et al., Monthly Not. Roy. Astron. Soc. 408, 16 (2010).</mixed-citation></ref><ref id="B111"><label>111.</label><mixed-citation>B. Cuevas-Otahola, Y. Mayya, I. Puerari et al., Monthly Not. Roy. Astron. Soc. 500, 4422 (2021).</mixed-citation></ref><ref id="B112"><label>112.</label><mixed-citation>M. Gieles, ASP Conf. Ser. 470, 339 (2013).</mixed-citation></ref><ref id="B113"><label>113.</label><mixed-citation>V. Jadhav, P. Kroupa, W. Wu, J. Pflamm-Altenburg, I. Thies, Astron. and Astrophys. 687, id.A89 (2024).</mixed-citation></ref><ref id="B114"><label>114.</label><mixed-citation>A.R. Shirazi, H. Haghi, A.H. Zonoozi, A. Farhani Asl, P. Kroupa, Monthly Not. Roy. Astron. Soc. 531, Issue 4, pp.4166 (2024).</mixed-citation></ref><ref id="B115"><label>115.</label><mixed-citation>M. Mezchua, H. Dominguez Sanchez, Monthly Not. Roy. Astron. Soc. 528, pp.5252 (2024).</mixed-citation></ref><ref id="B116"><label>116.</label><mixed-citation>M. Figueira, M. Siudek, A. Pollo, et al. Astron. and Astrophys. 687, id.A117 (2024).</mixed-citation></ref><ref id="B117"><label>117.</label><mixed-citation>A. Tokovinin, Astrophys. J. Supp. Ser. 235, 6 (2018).</mixed-citation></ref><ref id="B118"><label>118.</label><mixed-citation>T. Merle, Bulletin de la Société Royale des Sciences de Liège 93, 170 (2024).</mixed-citation></ref><ref id="B119"><label>119.</label><mixed-citation>X. Pang, Y. Li, Z. Yu et al., Astrophys. J. 912, 162 (2021).</mixed-citation></ref><ref id="B120"><label>120.</label><mixed-citation>A. Tutukov, S. Vereshchagin, Physics-Uspekhi 66, 859 (2023).</mixed-citation></ref><ref id="B121"><label>121.</label><mixed-citation>R. Ibata, K. Malhan, N. Martin et al., Astrophys. J. 914, 123 (2021).</mixed-citation></ref><ref id="B122"><label>122.</label><mixed-citation>L. Bai, J. Zhong, L. Chen, J. Li, J. Hou, Research in Astron. and Astrophys. 22, id.055022 (2022).</mixed-citation></ref><ref id="B123"><label>123.</label><mixed-citation>K.V. Nedkova, M. Rafelski, H.I. Teplitz, V. Mehta, et al., Astrophys. J. 970, id.188 (2024).</mixed-citation></ref><ref id="B124"><label>124.</label><mixed-citation>M. Kulesh, A. Samirkhanova, G. Carraro, et al., Astron. J. 167, id.212 (2024).</mixed-citation></ref></ref-list></back></article>
