MS
Main sequence star (hydrogen core burning).
Giant
Giant star (hydrogen core exostion).
Be
Be-star. Massive star after the accretion of the matter of its more massive companion.
WR
Wolf-Rayet star. Hydrogen envelope is lost after the common envelope stage. Be careful, we use evolutionary criterion, not the observational one! Single WR-stars are not formed in our scenario.
TZ
Thorne-Zytkow object. Neutron star inside a supergiant star.
SN Remn
Supernova remnant.
Planet
Planet (low-massive object: M<0.08 M_solar).
RLO(MB)
Roche lobe overflow due to magnetic stellar wind.
RLO(WR)
Roche lobe overflow by the Wolf-Rayet star.
RLO(GR)
Roche lobe overflow under the influence of the gravitational waves radiation.
RLO(WD)
Roche lobe overflow by the White Dwarf.
RLO(short)
Roche lobe overflow before the common envelope stage. Very short stage.
RLO(fast)
Roche lobe overflow in the dynamical timescale.
RLO(slow)
Roche lobe overflow in the thermal timescale.
Hot WD
Hot White Dwarf.
WD "E"
White dwarf in the regime of Ejector. Stopping radius greater than light cylinder radius.
WD "P"
White dwarf in the regime of Propeller. Co-rotation radius greater than stopping radius.
WD "A"
White dwarf in the regime of Accretor. Co-rotation radius less than stopping radius and stopping radius is less than gravitational capture radius.
WD "G"
White dwarf in the regime of Georotator. Stopping radius radius is greater than gravitational capture radius.
WD "SE"
White dwarf in the regime of SuperEjector. Ejector regime with companion Roche-lobe overflow.
WD "SP"
White dwarf in the regime of SuperPropeller. Propeller regime with companion Roche-lobe overflow.
WD "SA"
White dwarf in the regime of SuperAccretor. Regime of accretion with superEddington accretion rate.
Magnetor
Magnetor.
PSR
Radio pulsar.
NS "E"
Neutron Star in the regime of Ejector. Stopping radius greater than light cylinder radius.
NS "P"
Neutron Star in the regime of Propeller. Co-rotation radius greater than stopping radius.
NS "A"
Neutron Star in the regime of Accretor. Co-rotation radius less than stopping radius and stopping radius is less than gravitational capture radius.
NS "G"
Neutron Star in the regime of Georotator. Stopping radius radius is greater than gravitational capture radius.
NS "SE"
Neutron Star in the regime of SuperEjector. Regime of Ejector, but companion fills its Roche-lobe. Neutron star is inside a cavity, around it a big envelope exist.
NS "SP"
Neutron Star in the regime of SuperPropeller. Regime of Propeller, but companion fills its Roche-lobe. Neutron star is inside a cavity, around it a big envelope exist.
NS "SA"
Neutron Star in the regime of SuperAccretor. Regime of accretion with superEddington accretion rate.
BH
Black Hole. Black hole is formed after collapse if initial stellar mass was greater than some critical value, determined by the user.
BH "SA"
Black Hole in the regime of SuperAccretor. Regime of accretion with superEddington accretion rate.
Mass.Disk
Massive disk. Before or after coalescence.
Bad Stage
Bad stage (error).
SN Ia
Supernova of the type Ia.
SN Ib
Supernova of the type Ib.
SN II
Supernova of the type II.
Coalescence
Coalescence of binary's companions.
Disruption
Disruption of the binary system. For example if more than 1/2 of matter is ejected from the system (in zero eccentrisity case).
SN->II
Black Hole formation after the supernova explosion.
Evaporation
Evaporation of the companion of the binary.
Pl.Neb
Planetary nebulae.
AIC WD
Accretion induced collapse of the White Dwarf.


This page was designed by
Sergey Nazin.
Send questions and comments to leng@sai.msu.su