Big Chemical Encyclopedia

Chemical substances, components, reactions, process design ...

Articles Figures Tables About

FU Orionis outbursts

FU Orionis outbursts the brightening of an FU Orionis star. Such outbursts are thought to occur when the mass accretion rate through the accretion disk increases by orders of magnitude. [Pg.353]

Accretion-Disk-Instability Model for Outbursts of FU Orionis... [Pg.240]

We consider the criterion for the validity of giving occasion to the recurrence outburst of FU Orionis in our model. As shown in Figure, there are three condition which must be satisfied for our model. (A) the viscosity due to the prescription of self-gravitational instabilities is higher than that of standard ot-disk prescription, v [Pg.241]

See other pages where FU Orionis outbursts is mentioned: [Pg.316]    [Pg.71]    [Pg.69]    [Pg.70]    [Pg.70]    [Pg.71]    [Pg.81]    [Pg.190]    [Pg.316]    [Pg.71]    [Pg.69]    [Pg.70]    [Pg.70]    [Pg.71]    [Pg.81]    [Pg.190]    [Pg.240]    [Pg.239]   
See also in sourсe #XX -- [ Pg.71 , Pg.239 ]



SEARCH



FU Orionis

Outbursts

© 2024 chempedia.info