BLACK HOLE PHYSICS;
CELESTIAL MECHANICS;
STELLAR DYNAMICS;
HYDRODYNAMICS;
D O I:
10.1086/173380
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Using a three-dimensional Eulerian hydrodynamical code we consider close encounters of a star with a massive black hole that are accompanied by stripping of matter from the star, or disruption of it. An estimate is made of the critical pericentric distance at which the deposited energy is equal to the binding energy of the stellar model. Stripping of the outer layers and strong squeezing of the star by tidal forces are discussed.
机构:
MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave,37-664H, Cambridge, MA 02139 USANorthwestern Univ, Dept Phys & Astron, 2145 Sheridan Rd, Evanston, IL 60208 USA
Rodriguez, Carl
Haster, Carl-Johan
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机构:
MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave,37-664H, Cambridge, MA 02139 USA
Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 3H8, Canada
LIGO Lab, 77 Massachusetts Ave,37-664H, Cambridge, MA 02139 USANorthwestern Univ, Dept Phys & Astron, 2145 Sheridan Rd, Evanston, IL 60208 USA
Haster, Carl-Johan
Ramirez-Ruiz, Enrico
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机构:
Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen O, DenmarkNorthwestern Univ, Dept Phys & Astron, 2145 Sheridan Rd, Evanston, IL 60208 USA