Not exact matches
HAWC researchers tested how positrons travel through space
by measuring gamma rays, or high - energy light, from two
nearby pulsars — Geminga and Monogem — around 900 light - years away.
«Our analysis does not support previous claims that the two
nearby pulsars are responsible for the excess of positrons detected
by two space - born telescopes, the Italian - lead PAMELA project and the AMS - 02 detector of NASA,» she says.
By catching and counting particles of light streaming from these
nearby stellar engines, the HAWC collaboration showed that the two
pulsars are unlikely to be the origin of the positron excess.
The size of this stellar debris field, measured
by the patch of sky that glows bright in gamma rays, tells researchers how quickly matter moves relative to a local astrophysical engine — in this case, the
nearby pulsars.
This star's capricious behavior appears to be fueled
by a
nearby companion star and may give new insights into the birth of millisecond
pulsars.
To find out whether the jets could be the result of a magnetic field produced
by charged ions swirling around in the gas, Eatough and colleagues looked at a
nearby pulsar.