Thin spherically radiating shells and astronomical collapsed objects (Q1356635)
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scientific article; zbMATH DE number 1018761
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Thin spherically radiating shells and astronomical collapsed objects |
scientific article; zbMATH DE number 1018761 |
Statements
Thin spherically radiating shells and astronomical collapsed objects (English)
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13 November 1997
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We explain the de-accelerated motion of the shock wave that moves from the star surface or near the black hole, towards the outer atmosphere and perhaps also to a shell of matter that is expelled from this atmosphere. We use a black hole but not a neutron star, because in the former the gravitational field is very important.
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stress-tensor
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spherical star atmosphere
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de-accelerated motion
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shock wave
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star surface
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gravitational field
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