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Open Astronomy

formerly Baltic Astronomy

Editor-in-Chief: Barbuy, Beatriz


IMPACT FACTOR 2018: 0.350

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Volume 23, Issue 3-4

Issues

On Cluster Rotation in the Galactic Tidal Field

Leonid P. Ossipkov
  • Department of Space Technologies and Applied Astrodynamics, Saint Petersburg State University, 35 Universitetskij pr., Staryj Peterhof, St. Petersburg 198504, Russian Federation
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Published Online: 2017-02-18 | DOI: https://doi.org/10.1515/astro-2017-0191

Abstract

The dynamics of a rotating star cluster moving along a circular orbit in the axisymmetrical steady Galaxy is considered. The generalized tensor virial theorem allows to estimate its rotation speed. Conditions for direct and retrograde rotation in the galactic plane are found.

Keywords: stellar dynamics; methods: analytical; globular clusters: general; open clusters and associations: general

REFERENCES

  • Bok B. 1934, Circ. Harvard Obs., 384, 1Google Scholar

  • Buliga S. D., Ossipkov L. P. 2011, Vestnik Udmurt. Univ., Ser. astron., math. & phys., 1, 61Google Scholar

  • Callandreau G. 1892, Ann. Observ. Paris, 20, B1Google Scholar

  • Callandreau G. 1902, Ann. Observ. Paris, 22, D1Google Scholar

  • Chandrasekhar S. 1942, Principles of Stellar Dynamics, Chicago University PressGoogle Scholar

  • Chandrasekhar S., Lee E. P. 1968, MNRAS, 139, 135Google Scholar

  • Cimino M. 1956, Atti Acad. Naz. Lincei. rend. Sc. fis. mat. e nat., 20, 217Google Scholar

  • Davydenko A. A. 2013, Vestnik Udmurt. Univ., Ser. math., mech. & comp. sci., 2, 59Google Scholar

  • Fessenkov V. G. 1951, AZh, 28, 492Google Scholar

  • Kondratiev B. P. 2001, in Stellar Dynamics: from Classic to Modern, ed. L. P. Ossipkov, I. I. Nikiforov, St. Petersburg, Sobolev Astron. Inst., p. 399Google Scholar

  • Kondratiev B. P., Trubitsina N. G. 2010, Vestnik Udmurt. Univ., Ser. astron., math. & phys., 1, 52Google Scholar

  • Kuzmin G. G. 1963, Publ. Tartu Obs., 34, 9Google Scholar

  • Kuzmin G. G. 1965, Trudy Astrofiz. Inst., Alma-Ata, 5, 70Google Scholar

  • Lee S.-W., Rood S. J. 1969, J. Korean Astron. Soc., 2, 1Google Scholar

  • Lowell P. 1911, AJ, 26, 171Google Scholar

  • Lowell P. 1912, Bull. Astron., 29, 94Google Scholar

  • Mayot B. 1945, Ann. d’Astrophys., 8, 43Google Scholar

  • Mineur H., 1939, Ann. d’Astrophys., 2, 1Google Scholar

  • Nezhinsky E. M., Ossipkov L. P. 1987, Astron. Tsirkuliar, 1477, 1Google Scholar

  • Ogorodnikov K. F. 1965, Dynamics of Stellar Systems, Pergamon Press, LondonGoogle Scholar

  • Ossipkov L. P. 1985, in Studies in Astronomy and Geodesy, ed. K. A. Barkhatova, Sverdlovsk, Ural Univ. Press, p. 9Google Scholar

  • Ossipkov L. P. 1993, Vestnik St. Petersburg Univ., Ser. 1 (math., mech. & astron.), 3, 125Google Scholar

  • Ossipkov L. P. 2000, Astrophysics, 43, 215Google Scholar

  • Ossipkov L. P. 2001, in Dynamics of Star Clusters and the Milky Way, ASP Conf. Ser., vol. 228, San Francisco, p. 341Google Scholar

  • Ossipkov L. P. 2003, in Mathematical Methods of Studying Space Systems, ed. V. N. Starkov, St. Petersburg, Faculty of Appl. Math. & Control Processes, St. Petersburg State University, p. 73Google Scholar

  • Ossipkov L. P. 2004, in Order and Chaos in Stellar and Planetary Systems, ASP Conf. Ser., vol. 316, San Francisco, p. 345Google Scholar

  • Ossipkov L. P. 2006, Astronomy Reports, 50, 116Google Scholar

  • Ossipkov L. P. 2007, Vestnik St. Petersburg Univ., Ser. 10 (appl. math., control proc. & informatics), 3, 62Google Scholar

  • Ossipkov L. P. 2014, Astron. Astrophys. Transactions, 28, iss. 4Google Scholar

  • Ossipkov L. P., Kutuzov S. A., Nezhinsky E. M., Ollongren A. 1997, in Studies in Astronomy and Geodesy. Some Problems of Observational Astronomy, Ural University Press, Ekaterinburg, p. 98.Google Scholar

  • Picart L. 1904, Ann. Obs. Bordeaux, 5, 1Google Scholar

  • Proskurin S. A., Ossipkov L. P. 2013, Vestnik Udmurt. Univ., Ser. math., mech. & comp. sci., 2, 116Google Scholar

  • Rein N. F. 1936a, Trudy Sternberg Astron. Inst., 9, 191Google Scholar

  • Rein N. F. 1936b, AZh, 13, 414Google Scholar

  • Roche E. 1859, Ann. Observ. Paris, 5, 1Google Scholar

  • Spitzer L. 1987, Dynamical Evolution of Globular Clusters, Princeton University PressGoogle Scholar

  • van Wijk U. 1949, Ann. d’Astrophys., 12, 81Google Scholar

About the article

Received: 2014-11-13

Accepted: 2014-11-24

Published Online: 2017-02-18

Published in Print: 2014-12-01


Citation Information: Open Astronomy, Volume 23, Issue 3-4, Pages 272–278, ISSN (Online) 2543-6376, DOI: https://doi.org/10.1515/astro-2017-0191.

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© 2014 Leonid P. Ossipkov, published by De Gruyter Open. This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License. BY-NC-ND 3.0

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