PULSARS CLASS ASTRONOMICAL OBJECTS SOURCES DISPLAYING STRICT VARIATIONS PERIODS RANGE LITTLE FRACTION PULSAR NEUTRON STAR IN ORBIT NORMAL STELLAR COMPANION TYPE BINARY STAR SYSTEM STRENGTH THE SURFACE TESLA TRILLION TIMES STRONGER MAGNETIC FIELD MEASURED THE EARTH GAS CHANNELED NEUTRON STARS MAGNETIC POLES SIMILAR AURORAL ZONES GAS CAN REACH HALF THE SPEED OF LIGHT SO MUCH GRAVITATIONAL POTENTIAL ENERGY SQUARE KILOMETER TEN THOUSAND LUMINOUS THE SUN TEMPERATURES MILLIONS EMIT PULSES MOVE OUT OF VIEW AXIS WITH RESPECT TO THE SPIN VARIETY DEPEND SIZE SHAPE ORBITAL PATH NATURE THE COMPANION STARS MASSIVE YOUNG SUPERGIANTS STELLAR CLASSIFICATION RADIATION DRIVEN STELLAR WIND IN THE WIND CAPTURES FLOWS NEARBY VELA EXAMPLE KIND ORBITS STRONG GRAVITATIONAL FORCE PULL MATERIAL THE COMPANIONS ATMOSPHERE ORBIT ITSELF MASS TRANSFER PROCESS ROCHE LOBE CAPTURED ACCRETION DISC SPIRALS FALL ONTO THE BINARY APPARENTLY SHEDS DISK COMPANIONS ELLIPTICAL CIRCUMSTELLAR DISK CAPTURE CONTRACTS UNKNOWN TRANSIENT MONTHS EPISODES OBSERVABLE RADIO PULSAR EXHIBIT SPIN BEHAVIORS CHARACTERISTIC ACCEPTED MANIFESTATIONS OF ROTATING ROTATION CYCLE CASES IDENTIFIED THE PULSE THE MAJOR DIFFERENCES RADIO PULSARS ON THE ORDER OF MILLISECONDS ANGULAR MOMENTUM SLOWING SPINNING FASTER SHOW CHANGE PULSE PERIOD DISPLAY EXPLANATION DIFFERENCE PHYSICAL RADIATE AWAY ROTATIONAL ENERGY RELATIVISTIC PARTICLE MAGNETIC DIPOLE LIGHTING NEBULAE SURROUND MATTER WINDS ACCRETION DISKS CAUSING RATE INCREASE DECREASE RATES HUNDREDS SPIN DOWN BEHAVIOR UNDERSTOOD SATELLITES LOW EARTH ORBIT OBSERVATIONS THE EARLY ASTRONOMY BALLOONS SOUNDING ROCKETS DISCOVERED CENTAURUS UHURU MAGNETAR MILLISECOND PULSAR PULSAR PLANETS