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Gravitational waves from neutron stars and asteroseismology
Neutron stars are born in the supernova explosion of massive stars. Neutron stars rotate as stably as atomic clocks and possess densities exceeding that of atomic nuclei and magnetic fields millions to billions of times stronger than those created in laboratories on the Earth. The physical propertie...
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| Published in: | Philos Trans A Math Phys Eng Sci |
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| Main Author: | |
| Format: | Artigo |
| Language: | Inglês |
| Published: |
The Royal Society Publishing
2018
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| Subjects: | |
| Online Access: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5915648/ https://ncbi.nlm.nih.gov/pubmed/29661975 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2017.0285 |
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