scholarly journals The distance variation due to mass transfer and mass loss in (13.6+8) Mand (13+10) M binary star systems

2019 ◽  
Vol 11 (20) ◽  
pp. 9-16
Author(s):  
Mohammed R. Abdulameer

In this research the change in the distance of the two stars in two binary star systems (13.6+8)M8and (13+10)M8 was studied, through the calculations the value  (rate of mass transfer) of the two phases of dynamical stages of mass which are mass loss and mass transfer has been extracted in its own way ,by extracting the value of  the value of (the distance variation between the two stars) has been found only in the mass transfer stage by using mathematical model ,in mass loss stage  and   were calculated from the change and the difference between the values of each at different times of binary star system evolution ,it was found that  the maximum values of  and  are in mass transfer state in binary star system , in other words the maximum values of  depend on the mass transfer between the two component stars of the binary star system.

1995 ◽  
Vol 439 ◽  
pp. 417 ◽  
Author(s):  
R. D. Gehrz ◽  
T. L. Hayward ◽  
J. R. Houck ◽  
J. W. Miles ◽  
R. M. Hjellming ◽  
...  

Nature ◽  
1942 ◽  
Vol 150 (3810) ◽  
pp. 545-545

Science ◽  
2014 ◽  
Vol 344 (6181) ◽  
pp. 275-277 ◽  
Author(s):  
E. Kruse ◽  
E. Agol

2014 ◽  
Vol 9 (S310) ◽  
pp. 86-87
Author(s):  
D. Bancelin ◽  
E. Pilat-Lohinger ◽  
S. Eggl ◽  
R. Dvorak

AbstractBy now, observations of exoplanets have found more than 50 binary star systems hosting 71 planets. We expect these numbers to increase as more than 70% of the main sequence stars in the solar neighborhood are members of binary or multiple systems. The planetary motion in such systems depends strongly on both the parameters of the stellar system (stellar separation and eccentricity) and the architecture of the planetary system (number of planets and their orbital behaviour). In case a terrestrial planet moves in the so-called habitable zone (HZ) of its host star, the habitability of this planet depends on many parameters. A crucial factor is certainly the amount of water. We investigate in this work the transport of water from beyond the snow-line to the HZ in a binary star system and compare it to a single star system.


2008 ◽  
Vol 387 (2) ◽  
pp. 481-496 ◽  
Author(s):  
N. J. Dunstone ◽  
G. A. J. Hussain ◽  
A. Collier Cameron ◽  
S. C. Marsden ◽  
M. Jardine ◽  
...  

2018 ◽  
Author(s):  
Salvador Barquin

Discovery of a new binary star system (GSC 03905-01870 = USNO-B1.0 1431-0327922 = UCAC4 716-059522) in the Draco constellation is presented. It was discovered during a search for previously unreported eclipsing binary stars through the ASAS-SN database. The shape of the light curve and its characteristics (period of 0.428988±0.000001 d, amplitude of 0.34±0.02 V Mag, primary minimum epoch HJD 2457994.2756±0.0002) indicates that the new variable star is an eclipsing binary of W Ursae Majoris type. I registered this variable star in The International Variable Star Index (VSX), its AAVSO UID is 000-BMP-891.


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