When the core of a massive star is compressed during a supernova explosion, then collapses into a neutron star, it retains most of its angular momentum.
Since it has only a tiny fraction of its original radius, a neutron star is formed with a very high rotational speed.
A pulsar is a highly magnetised, dense neutron star emitting a beam of electromagnetic radiation.
The astronomer's observations proved that cephid variable stars would pulsate in a regular cycle
Cepheid Variables.
RR Lyrae variables are variable stars often used as standard candles. RR Lyrae are pulsating horizontal branch stars.
The pulsating spots, often seen in various celestial bodies or phenomena, can be attributed to changes in brightness or energy output. In stars, for instance, pulsations can result from internal processes such as thermal expansion and contraction, leading to varying surface temperatures and luminosities. In other contexts, like certain types of nebulae or variable stars, pulsations may be caused by gravitational forces or energy fluctuations within the object. These dynamic changes create a visual effect of pulsating light or color.
A pulsating star is a type of variable star that changes in brightness due to periodic expansions and contractions of its outer layers. These changes can be regular or irregular, and the star's size and temperature vary over time. Examples of pulsating stars include Cepheid variables and RR Lyrae stars.
Pulsars have extremely short periods; in some cases seconds, in some cases just a few milliseconds. There is no way a typical star, with its great size (for example, a diameter of 1.4 million kilometers in the case of our Sun) can pulsate that quickly.
Pulsating variable stars are stars that undergo periodic changes in brightness due to expansions and contractions in their outer layers. This rhythmic pulsation is primarily caused by instabilities in their stellar atmospheres, often linked to processes such as the ionization of helium. Common examples include Cepheid variables and RR Lyrae stars, which are crucial for measuring cosmic distances. Their predictable brightness variations make them important tools in astrophysics for understanding the scale of the universe.
A Cepheid is a member of a class of pulsating variable stars. The relationship between a Cepheid variable's luminosity and pulsation period is quite precise, securing Cepheids as viable standard candles and the foundation of the Extragalactic Distance Scale.
mooohiytsert
A pulsating star is a type of variable star that undergoes periodic changes in brightness due to expansions and contractions in its outer layers. Examples include Cepheid variables and RR Lyrae stars, which exhibit regular cycles of brightness changes. These stars are important for measuring cosmic distances, as their pulsation periods are directly related to their intrinsic luminosities.
There are two types of "pulsating" stars. 1. Pulsar 2. Quasar A pulsar is actually a neutron star that is rotating at a fast rate and is releasing a jet of X-rays. So, to a special telescope, it appears to be pulsating A quasar is similar to a pulsar, except for being a neutron star, it is a black hole.
No, they are completely different. See related questions