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In astronomy, an intermediate polar (also called a DQ Herculis Star) is a type of cataclysmic variable, binary star system with a white dwarf and a cool main-sequence secondary star. In most cataclysmic variables, matter from the companion star is gravitationally stripped by the compact star and forms an accretion disk around it. In intermediate polar…
Physical Properties, Light curve periodicities & Overview
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white intermediate dwarf polar magnetic systems cataclysmic field accretion disk variable star herculis polars may called 2006 light curve system
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Intermediate polar | is a | existence of a spin period signal that is shorter than the orbital period | 0.90 | text |
| Intermediate polar | related to External links | The Intermediate Polars | 0.60 | section |
| Intermediate polar | related to External links | Retrieved May | 0.60 | section |
| Intermediate polar | related to External links | Nemiroff | 0.60 | section |
| Intermediate polar | related to External links | Bonnell | 0.60 | section |
| Intermediate polar | related to External links | November | 0.60 | section |
| Intermediate polar | related to External links | An Intermediate Polar Binary | 0.60 | section |
| Intermediate polar | related to External links | System | 0.60 | section |
| Intermediate polar | related to External links | Astronomy Picture | 0.60 | section |
| Intermediate polar | related to External links | Day | 0.60 | section |
| Intermediate polar | related to External links | NASA | 0.60 | section |
| Intermediate polar | related to Light curve periodicities | The | 0.60 | section |
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