This beautiful supernova remnant and pulsar can be found between Taurus and Cygnus. Recently discovered, it lies at a distance of 6000 ly, and is believed to be the remnant of a Wolf-Rayet star, which probably went supernova about 7000 years ago.

The image is a Crowd Image. It was made, by combining 291 different amateur photos.

Image credits (Thanks for sharing your work! ;)

Adam Evans, Álvaro Pérez Alonso, Alvin, Alvinillo, Andolfato, Andrea Pistocchini, AstroGG, ASTROIDF, Astroluc63, Ben Gilsrud, Besnier.m, Bob WInter, bossakungen, budman1961, Burkhard, Carsten Frenzl, Carsten Frenzl, chaddkn, chripell, Chris Madson, Claustonberry, Cody Garges, Creedence, Dan, Dan Watt, Daniele Malleo, Danny Flippo, dave halliday, dave halliday, David Warrington, Davide Simonetti, Dominic Reeve, Eric Gorski, Ferran Ginebrosa, Flavastro, Florian Schlagintweit, fragro, Francesco di Biase, FranckIM06, Frank Zoltowski, Fred Locklear, Fredéric Segato, Fryns, Gaby, galaad16, geco71, Giuliano Pinazzi, Haim Huli, Hewholooks, Ian Papworth, J.Mattei, James Abbott, Jan Curtis, Jason Tackett, JeffJohnson, Jeremy, Jjstott, John Carruthers, jose, jpstanley, jpstanley, Jschulman555, JSpower, Juan Lozano, Judith Selig, Jürgen Kemmerer, Jussi Kantola, Ken_Lord, Kevin Heider, lacomj, lizarranet, Ljubinko Jovanovic, Luc Jamet, Luca Argalia, Manuel Orsatti, Marc Van Norden, Marcelo Domingues, maxgaspa, Michael F. Schönitzer, Michael Karrer, Michael Southam, Michele Fabrizio, Michele Palma, Mike Durkin, Miodrag Sekulic, Morten Balling, neptun, NicolasP, Olivier x, pascvale13, Paul Cotton, Paul M. Hutchinson, Pavel (sypai) Syrin, Peleg Wasserman, pfile, Phil Hosey, Phillip Seeber, Piotr Ambroziak, Ram Viswanathan, Richie Jarvis, Richie Jarvis, Rob glover, robbeh, Rodrigo Cunha, Rusty Mayhew, s58y, Salvatore Iovene, Salvopa, Shane Poage, simonct, Stan McQueen, Stefano Giardinelli, Stephen Rahn, Steve, Steve Yan, stevebryson, theilr, Tim, Tim Powell, Tom Harrison, Tom Munnecke, Ubi Desperare Nescio, Valts Treibergs, Vegantares, Vincent Bhm, Walliang Jacques, Werner Mehl, zemt-fr.

Ps. It's amazing how the shapes of the two original nebulae resemble each other. Also the Ha lies within the soft OIII bubbles. Both even have strange dark bubble nebulae within the bright areas.

Version B is the M1 image and C is the Crescent image used to make this composite of both nebulae mixed together.