2D AND 3D MASS TRANSFER SIMULATIONS IN LYRAE SYSTEM

Автор(и)

  • V. V. Nazarenko Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 65014, Ukraine, Україна
  • L. V. Glazunova Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 65014, Ukraine, Україна
  • V. G. Karetnikov Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 65014, Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2001.14.99473

Ключові слова:

Stars, interact binary systems, simulation.

Анотація

2D and 3D mass transfer simulations of the mass transfer in β Lyrae binary system. We have received that from a point L3 40 percent of mass transfer from L1-point is lost. The structure of a gas envelope, around system is calculated. 3-D mass transfer simulations has shown presence the spiral shock in the disk around primary star's and a jet-like structures (a mass flow in vertical direction) over a stream.

Посилання

Belotserkovskii O.M., Davydov Yu.M.: 1982, "The big particles code in gas dynamics", Moskaw, Scientist

Bisikalo D.V., Boyarchuk A.A., Chechetkin V.M., Kuznetsov O.A., Molteni D.: 1999, Astron. Reports, 43, 797

Bisikalo D.V., Harmanec P., Boyarchuk A.A., Kuznetsov O.A., Hadrava P.: 2000, As.Ap., 353, 1009

Harmanec P., Morand F., Bonneau D., et al.: 1996, As.Ap., 312, 879

Hubeny L., Plaves M.J.: 1991, A.J., 102, 1156

Kurucz R.L.: 1979, Astrophys.J.Suppl.Ser., 40, 1

Lubow S.YH., Shu F.H.: 1975, Ap.J., 198, 383

Molteni D., Belvedere G., Lanzafame G.: 1991, MNRAS, 249, 748

Wilson R.E.: 1974, Ap.J., 189, 319

##submission.downloads##

Опубліковано

2017-04-20

Номер

Розділ

Статті