Supernova remnants represent the residual effects of massive stars which have reached the end of their life-cycle,
including a massive stellar explosion as a grand finale, and which leave behind them spectacular gas clouds and
stellar remnants (neutrinos) which cover multiple full moons in width across the sky. Regrettably, for residents
of the northern hemisphere, only four supernova remnants (SNR) are visible and, more specifically, the Crab Nebula (M1)
in Taurus, the massive Veil complex (NGC 6960, 6974, 6979, 6992, 6995) in Cygnus, the Jellyfish Nebula (IC 433) in
Gemini and Simeis 147 (aka Shajn 147, Sh 2-240) also in Taurus. The most recognized supernova remnant is perhaps the
Crab nebula in Taurus which is believed to have exploded in 1054 AD as documented by Chinese astronomers of the time
whereas Simeis 147 is especially dim and represents one of the faintest objects in the sky.
Note: An area approximately three square degrees just to the south of å-Cyg (mag 2.46) hosts
one of the most dramatic examples of a supernova remnant. Commonly referred to as the Veil Complex due to multiple large
areas of nebulosity, the area is characterized with an extended remnant to the east comprised of NGC 6992, 6995 and
IC1340; a central remnant comprised of NGC 6974, 6979 and
Simeis 3-188 (Pickering's Triangle); and the western remnant surrounding 52-Cyg
(mag 4.22) and catalogued as NGC 6960. Herschel was the first to discover the various nebulosities in 1825 and who treated
them as independent entities and, hence, for the various NGC assignments. The Veil complex is 1400 to 2600 light-years away
and spans another 50 light-years in diameter. It is very difficult to see naked eye but trivial with a modest telescope and
an O-III filter which reveals tremendous filamentary detail and interwined wisps of nebulosity. It is believed that this SNR
is a from a star which exploded 5000 to 8000 years ago.
Please click on the image below to display in higher resolution (900 x 1200)