instability strip造句
例句與造句
- These stars cross the instability strip and undergo very regular pulsations.
- When these stars cross the instability strip they will pulsate as short period Cepheids.
- Delta Scuti variables are found roughly where the classical instability strip intersects the main sequence.
- Very massive stars never cool sufficiently to reach the instability strip and do not ever become Cepheids.
- They lie near the instability strip, cooler than type I Cepheids more luminous than type II Cepheids.
- It's difficult to find instability strip in a sentence. 用instability strip造句挺難的
- Throughout their lifetime Delta Scuti stars exhibit pulsation when they are situated on the classical Cepheid instability strip.
- Post-AGB stars are believed to pulsate as RV Tauri variables when they cross the instability strip.
- The first instability strip crossing occurs rapidly during the transition from the main sequence to becoming a red supergiant.
- Other classes of unstable main-sequence stars, like Beta Cephei variables, are unrelated to this instability strip.
- These stars will cross the instability strip more than once and pulsate as Type I ( Classical ) Cepheid variables.
- Their pulsations are related to the same helium instability strip on the Hertzsprung Russell diagram as that of classical Cepheids.
- On the AGB, thermal pulses from the helium fusing shell may cause a blue loop across the instability strip.
- 14 Persei has been calculated to lie within the Cepheid instability strip although it is not considered to be variable.
- Uncertainty in the absolute magnitude means that the star may actually lie near the instability strip but not on it.
- In some cases, stars may cross the instability strip for a fourth and fifth time when helium shell burning starts.
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