- A
pulsar wind
nebula (PWN,
plural PWNe),
sometimes called a
plerion (derived from the Gr**** "πλήρης", pleres,
meaning "full"), is a type of
nebula sometimes...
- polarization,
which is
characteristic of a
pulsar or
plerion wind nebula. The
expansion speed of this
plerion is
approximately 1000 km/s. X-ray observations...
-
Intergalactic Dust
Medium ORCs
Nebulae Emission Planetary Supernova remnant Plerion H II
region Reflection Dark
nebulae Molecular cloud Bok
globule Proplyd...
-
centrally peaked and a very soft X-ray s**** is
barely visible.
Unlike plerion remnants, e.g. the Crab Nebula, the
inner X-ray
emission is not dominated...
-
synchrotron emission is
important is
pulsar wind nebulae, also
known as
plerions, of
which the Crab
nebula and its ****ociated
pulsar are archetypal. Pulsed...
- Weiler, K. W.; Panagia, N. (October 1980). "Vela X and the
Evolution of
Plerions".
Astronomy and Astrophysics. 90 (3): 269–282. Bibcode:1980A&A....90..269W...
-
between the two objects. Likewise, the
direction and
morphology of the
plerion tail
suggests a
physical connection between PSR J0002+6216 and CTB 1. The...
-
Dhyana for
viola d'amore and
piano Akhkhazu for alto
saxophone and
piano Plerion for
trumpet and
piano Tiamat for violin, viola, cello,
double b****, and...
-
Astrophysical Journal; 25
September 2002: [3]
Inhomogeneous models for
plerions: the
surface brightness profile of the Crab Nebula; E. Amato, M. Salvati...
