| 1. | Many of us are trying to predict their properties at this moment
至今，天文学家还在摸索著磁星的特质。 |
| 2. | With such a high magnetic field , magnetar slows down very rapidly
由于磁星的磁场非常强，它的减速率很高。 |
| 3. | This is where a magnetic field changes shape and bumps into itself
这就是磁星的磁场改变了形状然后向本身内部撞击。 |
| 4. | Concept image of a magnetar which is the object with the strongest magnetic field
构想的磁星是拥有最强磁场的天体。 |
| 5. | Magnetars , soft gamma repeaters very strong magnetic fields , robert c . duncan
磁星继发软伽玛射线源及极强磁场，邓肯 |
| 6. | In this respect , we are very lucky to find one and still the only one at this moment - sgr1806 - 20 - in the sky
然而sgr1806 - 20却被侥幸找到，亦是迄今唯一被发现的磁星。 |
| 7. | Owing to its super - strong magnetic field , calculating various properties of magnetars are hard problems for astronomers
磁星的磁场非常强，对天文学家来说，找出它们的特性绝非容易。 |
| 8. | Therefore soon after their supernova birth , their rotational speed will become so low that they stop to emit electromagnetic pulses
因此，超新星爆发后不久，磁星的自转速度会变得非常缓慢，因而停止发放电磁脉冲。 |
| 9. | We now call this kind of super - strong magnetic field neutron stars magnetar , a term coined a few years ago by two theoretical astrophysicists duncan and thompson
天体物理学家邓肯和汤逊在多年前已把这类具有超级强力磁场的中子星称为磁星。 |
| 10. | In other words , astronomers can only detect those extremely young energetic magnetars before they stop emittng electromagnetic pulses . consequently , it is extremely hard for us to find them in the sky
换句话说，天文学家只能向那些仍未停止发放电磁脉冲的年青有活力的磁星埋手，故此要在天空中寻找磁星非常困难。 |
