The ecology of rotators (Q1822577)
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scientific article; zbMATH DE number 4001724
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | The ecology of rotators |
scientific article; zbMATH DE number 4001724 |
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The ecology of rotators (English)
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1987
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The paper summarizes a special class of astrophysical objects: rotating bodies. They are characterized by three parameters: mass, magnetic field and angular momentum. The concept of the rotator is a useful theoretical tool for describing neutron stars, white duals, magnetic stars, supermassive stars (spinars) or active galactic nuclei. The rotator interacts with its environment via electromagnetic and gravitational fields. A general classification and formulae for a multitude of possible cases are presented.
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rotating bodies
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angular momentum
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rotator
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neutron stars
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white duals
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magnetic stars
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supermassive stars
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spinars
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active galactic nuclei
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gravitational fields
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classification
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0.78621984
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0.77623355
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0.77583486
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0.74927974
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0.74412584
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