Canon 350D Hap Griffin Baader Mod32x360sec at iso 1600
30 Darks/Flats/Bias
APM/TMB 130/780Astronomik CLS Front "Clip" FilterPLUS
Canon 350D Hap Griffin Baader Mod11x600sec at iso 1600
APM/TMB 130/780Baader 7nm H alpha filter
This image with the addition of
2 hours Ha data and combined with the
Starizona Method 2 where stars are diminished and nebulosity is increased. Then a top layer the original RGB as a "lighten" layer at 55% to add back some stars that are removed by the above method.
This object, or at least the nebulosity, was very challenging to image, but it was so interesting that I had to try it. I should have suspected it to be a tough target when Robert Gendler got
this out of it with a 20 inch RCOS and an SBIG STL-11000XM on a Paramount ME.
NGC 6820 is an emission nebula that surrounds open cluster NGC 6823 in Vulpecula, near M27, the Dumbbell nebula. The center of the open cluster formed only about two million years ago and is dominated in brightness by a host of
bright young blue stars. Outer parts of the cluster intimately involving pillars of emission nebula NGC 6820, contain even younger stars. The
huge pillars of gas and
dust likely get their elongated shape by
erosion from hot radiation emitted from the brightest cluster stars. Striking
dark globules of gas and dust are also visible in the nebula. Open star cluster
NGC 6823 spans about 50 light years and lies about 6000
light years away
July1 and July 14, 2008