Pseudo-Schwarzschild description of accretion-powered spherical outflow
| dc.contributor.author | Das, Tapas K. | |
| dc.date.accessioned | 2012-03-14T05:10:33Z | |
| dc.date.available | 2012-03-14T05:10:33Z | |
| dc.date.issued | 2001-07-02 | |
| dc.description.abstract | Using two different pseudo-Schwarzschild potentials proposed by Artemova et. al, 1 we formulate and solve the equations governing spherically symmetric transonic inflow and outflow in presence of a relativistic hadronic pressure mediated steady, standing, spher- ical shock around the central compact object and then we self-consistently connect the accretion-wind solutions to calculate the mass outflow rate R ˙ m in terms of minimum number of flow parameters. Also we study the dependence of this rate on various bound- ary conditions governing the flow. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/1482 | |
| dc.language.iso | en | en_US |
| dc.relation.ispartofseries | IUCAA Preprints;41/01 | |
| dc.subject | Pseudo-Schwarzschild description | en_US |
| dc.subject | Ccretion-powered spherical outflow | en_US |
| dc.title | Pseudo-Schwarzschild description of accretion-powered spherical outflow | en_US |
| dc.type | Article | en_US |