The BinaryStar object

The BinaryStar object is composed of two SingleStar objects and contains the current and past states of the binary. Only parameters in the BINARYPROPERTIES list are stored in the history. The current parameter value of the star object is accessed as, e.g. binary.orbital_period while his past history with binary.orbital_period_history. The two stars are accesses as, e.g. binary.star_1.mass while his past history with binary.star_1.mass_history.

To use BinaryStar object import it using:

from posydon.binary_evol.singlestar import SingleStar
from posydon.binary_evol.binarystar import BinaryStar

Creating a BinaryStar object

BINARYPROPERTIES

The binary properties are defined as follows

BINARYPROPERTIES

Properties

Descriptions

state

The state of the binary, see state options.

event

The event of the binary, see event options.

time

Age of the binary system in yr.

separation

Orbital separation in R_sun.

orbital_period

Orbital period in days.

eccentricity

Orbital eccentricity.

V_sys

Velocity of the centre of mass of the binary [Vx, Vy, Vz] in km/s.

mass_transfer_case

Mass transfer case, see MT case options.

TODO: add missing properties

State options

Binary states are defined according to the following table:

States

State

Description

detached

The stars in the binary are in a detached state.

contact

The stars in the binary are in contact.

RLO1

The binary is Roche Lobe overflowing, star 1 is overfilling the RL.

RLO2

The binary is Roche Lobe overflowing, star 2 is overfilling the RL.

CE

The binary is in a Common Envelope phase.

disrupted

The binary was disrupted.

MaxTimeChanged

Max time of the evolution was reached.

TODO: update properties

Event options

Binary events are defined according to the following table:

Events

State

Description

CC1

Core collapse of star 1.

CC2

Core collapse of star 2.

oRLO1

The binary is at onset of Roche Lobe overflow, star 1 is overfilling the RL.

oRLO2

The binary is at onset of Roche Lobe overflow, star 2 is overfilling the RL.

oCE

The binary is at the onset of Common Envelope.

None

No event occurred.

END

The binary evolution was stopped.

TODO: update properties

Mass Transfer case

The mass transfer cases are stored in mt_history_GRIDTYPE and are defined according to the following table: TODO: add the table below

Mass transfer cases

State

Description

None

The binary is not Roche Lobe overflowing.

TODO: update properties

Basic example

The simplest method is to provide the two star objects and kwargs of the initial binary parameters.

kwargs1 = {'state' : 'MS',
           'mass' : 20.0,
           'metallicity' : 0.014}

star_1 = SingleStar(**kwargs1)

kwargs2 = {'state' : 'MS',
           'mass' : 10.0,
           'metallicity' : 0.014}

star_2 = SingleStar(**kwargs2)

kwargs3 = {'state' : 'detached',
           'event' : None,
           'time' : 0.,
           'orbital_period' : 3.,
           'eccentricity' : 0.}


binary = BinaryStar(star_1, star_2, **kwargs3)