TWO SCENARIOS OF MASS EXCHANGE IN CLOSE BINARY SYSTEMS CONSISTING OF THE LOW MASS PRE-MAIN SEQUENCE STARS
In this paper, we present the results of smoothed particle hydrodynamic (SPH) simulations of mass transfer in close binary systems consisting of the low mass pre-main sequence stars. Two scenarios of mass exchange in such systems are possible. If the more massive component is closer to fill its Roch...
Main Author: | F. V. Sirotkin |
---|---|
Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2017-03-01
|
Series: | Odessa Astronomical Publications |
Online Access: | http://oap.onu.edu.ua/article/view/93263 |
Similar Items
-
THE PROTOPLANETARY SYSTEM FORMATION AS A RESULT OF THE MERGING OF CLOSE BINARY STAR CONSISTING OF THE LOW MASS PRE-MS STARS
by: F. V. Sirotkin, et al.
Published: (2017-04-01) -
PRE-MAIN SEQUENCE EVOLUTIONS OF SOLAR ABUNDANCE LOW MASS STARS
by: Youn Kil Jung, et al.
Published: (2007-03-01) -
Asteroseismology of Close Binary Stars: Tides and Mass Transfer
by: Zhao Guo
Published: (2021-05-01) -
DETERMINATION OF THE AGE OF LOW-MASS CLOSE BINARY STARS OF EARLY SPECTRAL CLASSES
by: I. I. Bondarenko, et al.
Published: (2017-04-01) -
MHD Modeling of Mass Transfer Processes in Close Binary Stars
by: Andrey Zhilkin, et al.
Published: (2022-12-01)