Автореферат (1145358), страница 6
Текст из файла (страница 6)
5. Отношение h/z0 как функцияMtot /Md для фильтра Ks . Незакрашенные квадраты — вся выборка, закрашенные квадраты — полная выборка.ностная яркость диска. На основе данных 2D декомпозиции для MSR10 выборки галактик, видимых с ребра, показано, что найденная корреляция являетсяложной (самокорреляцией) и возникает из-за применения формул редукции, переводящих наблюдаемую центральную поверхностную яркость µ0,d в депроецированную S0,d с использованием отношения z0 /h. На искусственных выборкахпродемонстрировано, при каких условиях может возникать такая самокорреляция. Вразделе 4.3приводятся выводы к четвертой главе.Результаты Главы 4 опубликованы в статьях [9, 10, 12, 19, 28, 29, 31].В Заключенииперечислены основные результаты, вошедшие в диссер-тационную работу.Список публикаций[1] Sotnikova N.
Y. Simulation of large-scale gas structures formed in the interaction between galaxies. I. Method and preliminary results // Astrophysics. 1996.Vol. 39. P. 141–152.[2] Reshetnikov V. P., Sotnikova N. Y. Global structure and formation of polar-ringgalaxies.
// A&A. 1997. Vol. 325. P. 933–942.[3] Sotnikova N. Y., Reshetnikov V. P. Tidal features as probes of dark matter ingalaxies // Bulletin of the Russian Academy of Sciences: Physics. 1998. Vol. 62.P. 1754–1758.[4] Sotnikova N. Y., Reshetnikov V. P. Star formation in the NGC-4676 system(the Mice) // Astronomy Letters. 1998. Vol. 24. P. 73–83.30[5] Reshetnikov V. P., Sotnikova N. Y.
The Polar Stellar Ring and Dark Halo ofNGC5907 // Astronomy Letters. 2000. Vol. 26. P. 277–284.[6] Reshetnikov V. P., Sotnikova N. Y. Tidal tails and galaxy evolution // Astronomical and Astrophysical Transactions. 2001. Vol. 20. P. 111–114.[7] Evstigneeva E. A., Reshetnikov V. P., Sotnikova N. Y. Numerical modelingof encounters between spherical galaxies // Stellar Dynamics: From Classic toModern, Proc. of the intern. conf.Saint-Petersburg, 2000 / Ed. by L. P. Ossipkov, I. I. Nikiforov. Saint-Petersburg: Sobolev Astronomical Institute, 2001.P.
162–165.[8] Evstigneeva E. A., Reshetnikov V. P., Sotnikova N. Y. Effect of the environmenton the fundamental plane of elliptical galaxies // A&A. 2002. Vol. 381. P. 6–12.[9] Sotnikova N. Y., Rodionov S. A. Mechanisms of the Vertical Secular Heatingof a Stellar Disk // Astronomy Letters. 2003. Vol. 29. P. 321–335.[10] Sotnikova N. Y., Rodionov S. A. Bending Instability of Stellar Disks: The Stabilizing Effect of a Compact Bulge // Astronomy Letters.
2005. Vol. 31. P. 15–29.[11] Rodionov S. A., Sotnikova N. Y. Optimal Choice of the Softening Length andTime Step in N-body Simulations // Astronomy Reports. 2005. Vol. 49.P. 470–476.[12] Sotnikova N. Y., Rodionov S. A. Estimating the dark halo mass from the relativethickness of stellar disks // Astronomy Letters. 2006. Vol. 32. P. 649–660.[13] Rodionov S. A., Sotnikova N. Y. An iterative method for the constructionof equilibrium N-body models for stellar disks // Astronomy Reports.
2006.Vol. 50. P. 983–1000.[14] Sotnikova N. Y., Grinin V. P. Hydrodynamic processes in young binaries asa source of cyclic variations in circumstellar extinction // Astronomy Letters.2007. Vol. 33. P. 594–603.[15] Sotnikova N. Y., Rodionov S. A. Anisotropic models of dark halos // AstronomyLetters. 2008. Vol. 34. P.
664–674.[16] Rodionov S. A., Athanassoula E., Sotnikova N. Y. The construction of equilib-31rium phase models of stellar systems by the iterative method // AstronomscheNachrichten. 2008. Vol. 329. P. 896–899.[17] Rodionov S. A., Athanassoula E., Sotnikova N.
Y. An iterative method forconstructing equilibrium phase models of stellar systems // MNRAS. 2009.Vol. 392. P. 904–916.[18] Sotnikova N. Y., Rodionov S. A. An iterative method for constructing stellarsystems models: how far does it work? // Highlights of Astronomy. 2010.Vol. 15. P. 203–203.[19] Mosenkov A. V., Sotnikova N. Y., P. R. V. 2MASS photometry of edge-on spiralgalaxies - I. Sample and general results // MNRAS. 2010. Vol. 401. P. 559–576.[20] Reshetnikov V. P., Moiseev A. V., Sotnikova N. Y.
Malin1: interacting galaxypair? // MNRAS. 2010. Vol. 406. P. L90–L94.[21] Demidova T. V., Sotnikova N. Y., Grinin V. P. Bimodal brightness oscillationsin models of young binary systems // Astronomy Letters. 2010. Vol. 36.P. 422–429.[22] Demidova T. V., Grinin V. P., Sotnikova N. Y.
Brightness oscillations in modelsof young binary systems with low-mass secondary components // AstronomyLetters. 2010. Vol. 36. P. 498–505.[23] Grinin V. P., Demidova T. V., Sotnikova N. Y. Modulation of circumstellar extinction in a young binary system with a low-mass companion in a noncoplanarorbit // Astronomy Letters. 2010. Vol. 36.
P. 808–815.[24] Silchenko O. K., Chilingarian I. V., Sotnikova N. Y., Afanasiev V. L. Large scalenested stellar discs in NGC 7217 // MNRAS. 2011. Vol. 414. P. 3645–3655.[25] Mohamed Y. H., Reshetnikov V. P., Sotnikova N. Y. On the characteristics oftidal structures of interacting galaxies // Astronomy Letters. 2011. Vol. 37.P. 670–678.[26] Sotnikova N. Y., Mosenkov A. V., Reshetnikov V.
P. Bulges and discs of spiralgalaxies: edge-on perspective // Astronomical and Astrophysical Transactions.2012. Vol. 27. P. 145–156.32[27] Demidova T. V., Grinin V. P., Sotnikova N. Y. Anisotropic illumination ofa circumbinary disk in the presence of a low-mass companion // AstronomyLetters. 2013. Vol. 39. P. 26–37.[28] Rodionov S.
A., Sotnikova N. Y. Bending instability in galactic discs: advocacyof the linear theory // MNRAS. 2013. Vol. 434. P. 2373–2379.[29] Bizyaev D. V., Kautsch S. J., Mosenkov A. V. et al. The Catalog of Edge-onDisk Galaxies from SDSS. I. The Catalog and the Structural Parameters ofStellar Disks // ApJ. 2014. Vol. 787. P. 24.[30] Sotnikova N. Y., Shapranov V. V. Tidal Stellar Loops and Dark Halo ofUGC 7388 // Multi-Spin Galaxies, ASP Conference Series / Ed. by E.
Iodice,E. M. Corsini. Vol. 486. 2014. P. 175–178.[31] Mosenkov A. V., Sotnikova N. Y., Reshetnikov V. P. Mirages in galaxy scalingrelations // MNRAS. 2014. Vol. 441. P. 1066–1085.Цитированная литература[1] Merritt D. Optimal Smoothing for N-Body Codes // AJ. 1996. Vol. 111.P. 2462–2464.[2] Chilingarian I. V., Prugniel P., Sil’Chenko O. K., Afanasiev V.
L. Kinematicsand stellar populations of the dwarf elliptical galaxy IC 3653 // MNRAS. 2007.Vol. 376. P. 1033–1046.[3] Le Borgne D., Rocca-Volmerange B., Prugniel P. et al. Evolutionary synthesisof galaxies at high spectral resolution with the code PEGASE-HR. Metallicityand age tracers // A&A. 2004. Vol. 425. P. 881–897.[4] Sil’chenko O. K., Afanasiev V. L. Decoupled nuclei and nuclear polar rings inregular spiral galaxies NGC 7217 // A&A.
2000. Vol. 364. P. 479–490.[5] Jog C. J., Solomon P. M. Two-fluid gravitational instabilities in a galacticdisk // ApJ. 1984. Vol. 276. P. 114–126.33[6] Efstathiou G. A model of supernova feedback in galaxy formation // MNRAS.2000. Vol. 317. P. 697–719.[7] Noordermeer E., van der Hulst J. M., Sancisi R. et al. The Westerbork HIsurvey of spiral and irregular galaxies.
III. HI observations of early-type diskgalaxies // A&A. 2005. Vol. 442. P. 137–157.[8] Toomre A. On the gravitational stability of a disk of stars // ApJ. 1964. Vol.139. P. 1217–1238.[9] Kennicutt R. C., Jr. The star formation law in galactic disks // ApJ.
1989.Vol. 344. P. 685–703.[10] Osipkov L. P. Spherical systems of gravitating bodies with an ellipsoidal velocitydistribution // Soviet Astronomy Letters. 1979. Vol. 5. P. 42–44.[11] Merritt D. Spherical stellar systems with spheroidal velocity distributions //AJ. 1985. Vol. 90.
P. 1027–1037.[12] Merritt D. Distribution functions for spherical galaxies // MNRAS. 1985. Vol.214. P. 25P–28P.[13] Navarro J. F., Frenk C. S., White S. D. M. The Structure of Cold Dark MatterHalos // ApJ. 1996. Vol. 462. P. 563–575.[14] Navarro J. F., Frenk C. S., White S. D. M. A Universal Density Profile fromHierarchical Clustering // ApJ. 1997. Vol. 490. P. 493–508.[15] Moore B., Quinn T., Governato F.
et al. Cold collapse and the core catastrophe // MNRAS. 1999. Vol. 310. P. 1147–1152.[16] Shang Z., Zheng Z., Brinks E. et al. Ring Structure and Warp of NGC 5907:Interaction with Dwarf Galaxies // ApJ. 1998. Vol. 504. P. L23–L26.[17] Toomre A., Toomre J. Galactic Bridges and Tails // ApJ. 1972. Vol. 178.P. 623–666.[18] Mihos J. C., Bothun G.
D., Richstone D. O. Modeling the Spatial Distributionof Star Formation in Interacting Disk Galaxies // ApJ. 1993. Vol. 418. P. 82–99.[19] Mapelli M., Moore B., Ripamonti E. et al. Are ring galaxies the ancestors ofgiant low surface brightness galaxies? // MNRAS.
![](https://s.studizba.com/z.php?f=/templates/si/i/noavatar.png&w=100&h=100&t=1"){kind=avatar}
