Azimuthal Patterns in Planetesimal Circumstellar Disks
- Authors: Demidova T.V.1,2, Shevchenko I.I.2,3
-
Affiliations:
- Crimean Astrophysical Observatory RAS
- St. Petersburg State University
- Institute of Applied Astronomy RAS
- Issue: Vol 49, No 6 (2023)
- Pages: 426-438
- Section: Articles
- URL: https://vestnikugrasu.org/0320-0108/article/view/674279
- DOI: https://doi.org/10.31857/S0320010823060025
- EDN: https://elibrary.ru/GNPSFO
- ID: 674279
Cite item
Abstract
Ways of formation of azimuthal resonant patterns in circumstellar planetesimal disks with planets are considered. Our analytical estimates and massive numerical experiments show that the disk particles that initially reside in zones of low-order mean-motion resonances with the planet may eventually concentrate into potentially observable azimuthal patterns. The structuring process is rapid, usually taking + 100 orbital periods of the planet. It is found that the relative number of particles that retain their resonant position increases with decreasing the mass parameter m (the ratio of masses of the perturbing planet and the parent star), but a significant fraction of the particle population is always removed from the disk due to accretion of the particles onto the star and planet, as well as due to their transition to highly elongated and hyperbolic orbits. Expected radio images of azimuthally structured disks are constructed. In the considered models, azimuthal patterns associated with the 2:1 and 3:2 resonances are most clearly manifested; observational manifestations of the 1:2 and 2:3 resonances are also possible.
About the authors
T. V. Demidova
Crimean Astrophysical Observatory RAS; St. Petersburg State University
Email: proxima1@list.ru
Nauchnyi, Russia; St. Petersburg, Russia
I. I. Shevchenko
St. Petersburg State University; Institute of Applied Astronomy RAS
Author for correspondence.
Email: proxima1@list.ru
St. Petersburg, Russia; St. Petersburg, Russia
References
- Агнор и др. (C.B. Agnor, R.M. Canup, and H.F. Levison), Icarus 142, 219 (1999).
- Бе и др. (H. Beust, J.-C. Augereau, A. Bonsor, J.R. Graham, P. Kalas, J. Lebreton, A.-M. Lagrange, S. Ertel, et al.), Astron. Astrophys. 561, A43 (2014).
- Борен, Хаффман (C.F. Bohren and D.R. Huffman), Absorption and Scattering of Light by Small Particles p. 544 (1998).
- ван дер Плас и др. (G. van der Plas, C.M. Wright, F. Ménard, S. Casassus, H. Canovas, C. Pinte, S.T. Maddison, K. Maaskant, et al.), Astron. Astrophys. 597, A32 (2017).
- Ваят (M.C. Wyatt), Ann. Rev. Astron. Astrophys. 46, 339 (2008).
- Ваят и др. (M.C. Wyatt, S.F. Dermott, C.M. Telesco, R.S. Fisher, K. Grogan, E.K. Holmes, and R.K. Piña), Astrophys. J. 527, 918 (1999).
- Ваят и др. (M.C. Wyatt, R. Smith, J.S. Greaves, C.A. Beichman, G. Bryden, and C.M. Lisse), Astrophys. J. 658, 569 (2007).
- Виздом (J. Wisdom), Astron. J. 85, 1122 (1980).
- Гаспар и др. (A. Gáspár, D. Psaltis, G.H. Rieke, and F. Özel), Astrophys. J. 754, 74 (2012).
- Гривз (J.S. Greaves), Science 307, 68 (2005).
- Даллемонд и др. (C.P. Dullemond, A. Juhasz, A. Pohl, F. Sereshti, R. Shetty, T. Peters, B. Commercon, and M. Flock), Astrophys. Source Code Library ascl:1202.015 (2012).
- Демидова (T. Demidova), Astron. Comput. 41, 100635 (2022).
- Демидова, Шевченко (T.V. Demidova and I.I. Shevchenko), Astrophys. J. 805, 38 (2015).
- Демидова, Шевченко (T.V. Demidova and I.I. Shevchenko), MNRAS 463, L22 (2016).
- Демидова Т.В., Шевченко И.И., Письма в Астрон. журн. 46, 827 (2020) [T.V. Demidova, I.I. Shevchenko, Astron. Lett. 46, 774 (2020)].
- Доминик, Дечин (C. Dominik and G. Decin), Astrophys. J. 598, 626 (2003).
- Донахи (J.S. Dohnanyi), J. Geophys. Res. 74, 2531 (1969).
- Доршнер и др. (J. Dorschner, B. Begemann, T. Henning, C. Jaeger, and H. Mutschke), Astron. Astrophys. 300, 503 (1995).
- Квиллен, Торндайк (A.C. Quillen and S. Thorndike), Astrophys. J. 578, L149 (2002).
- Квиллен (A.C. Quillen), MNRAS 372, L14 (2006).
- Квиллен, Фабер (A.C. Quillen and P. Faber), MNRAS 373, 1245 (2006).
- Кондратьев (B.P. Kondratyev), MNRAS 442, 1755 (2014).
- Кривов и др. (A.V. Krivov, I. Mann, and N.A. Krivova), Astron. Astrophys. 362, 1127 (2000).
- Кривов и др. (A.V. Krivov, T. Löhne, and M. Sremčević), Astron. Astrophys. 455, 509 (2006).
- Кривов (A.V. Krivov), Res. Astron. Astrophys. 10, 383 (2010).
- Кюхнер, Хольман (M.J. Kuchner and M.J. Holman), Astrophys. J. 588, 1110 (2003).
- Лене и др. (T. Löhne, A.V. Krivov, and J. Rodmann), Astrophys. J. 673, 1123 (2008).
- Лумис и др. (R.A. Loomis, K.I. Öberg, S.M. Andrews, and M.A. MacGregor), Astrophys. J. 840, 23 (2017).
- Львов и др. В.Н. Львов, Р.И. Смехачева, С.С. Смирнов, С.Д. Цекмействер, Изв. ГАО РАН 217, 318 (2004).
- Марино (S. Marino), arXiv e-prints arXiv:2202.03053 (2022).
- Ми (G. Mie), Annalen der Physik 330, 377 (1908).
- Моррисон, Мальхотра (S. Morrison and R. Malhotra), Astrophys. J. 799, 41 (2015).
- Мустилл, Ваят (A.J. Mustill and M.C. Wyatt), MNRAS 419, 3074 (2012).
- Мюррей, Дермотт (C.D. Murray and S.F. Dermott), Solar System Dynamics (Cambridge Univ. Press, 1999) [Мюррей К., Дермотт С., Динамика Солнечной системы (М.: Физматлит, 2009, 2010.)].
- Озерной и др. (L.M. Ozernoy, N.N. Gorkavyi, J.C. Mather, and T.A. Taidakova), Astrophys. J. 537, L147 (2000).
- Петри и др. (D. Petry and CASA Development Team), Astron. Data Analys. Software and Systems XXI 461, 849 (2012).
- Пирс, Ваят (T.D. Pearce and M.C. Wyatt), MNRAS 443, 2541 (2014).
- Питиева Е.В., Питиев Н.П., Письма в Астрон. журн. 44, 604 (2018а) [E.V. Pitjeva and N.P. Pitjev, Astron. Lett. 44, 554 (2018)].
- Питиева, Питиев (E.V. Pitjeva and N.P. Pitjev), Celestial Mechanics and Dynamical Astronomy 130, 57 (2018б).
- Пресс и др. (W.H. Press, S.A. Teukolsky, W.T. Vetterling, and B.P. Flannery) Numerical recipes in C. The art of scientific computing (Cambridge University Press, 1992), p. 724.
- Родигас и др. (T.J. Rodigas, R. Malhotra, and P.M. Hinz), Astrophys. J. 780, 65 (2014).
- Руге и др. (J.P. Ruge, S. Wolf, T. Demidova, and V. Grinin), Astron. Astrophys. 579, A110 (2015).
- Савин и др. (G.I. Savin, B.M. Shabanov, P.N. Telegin, and A.V. Baranov), Lobachevskii J. Math. 40, 1853 (2019).
- Су и др. (K.Y.L. Su, G.H. Rieke, R. Malhotra, K.R. Stapelfeldt, A.M. Hughes, A. Bonsor, D.J. Wilner, Z. Balog, et al.), Astrophys. J. 763, 118 (2013).
- Тебо, Ожеро (P. Thébault and J.-C. Augereau), Astron. Astrophys. 472, 169 (2007).
- Тейлор (S.R. Taylor), Meteorit. Planet. Sci. Suppl. 33, A153 (1998).
- Феделе и др. (D. Fedele, M. Carney, M.R. Hogerheijde, C. Walsh, A. Miotello, P. Klaassen, S. Bruderer, Th. Henning, et al.), Astron. Astrophys. 600, A72 (2017).
- Чемберс, Уэтерилл (J.E. Chambers and G.W. Wetherill), Icarus 136, 304 (1998).
- Шевченко (I.I. Shevchenko), Astrophys. Space Sci. 463, 1 (2020).
- Штер, Булирш (J. Stoer and R. Bulirsch), Introduction to Numerical Analysis (Springer-Verlag, 1980).
- Эндрюс и др. (S.M. Andrews, D.J. Wilner, E. Macías, C. González, and A. Isella), Science with a Next Generation Very Large Array 517, 137 (2018).
Supplementary files
