Placidus
31-05-2016, 06:27 PM
Our goal here was to capture some of the really faint detail in the Bug Nebula, that is not normally shown in amateur images.
Hubble palette, but with stars whitened. 0.55 sec arc/pixel. FOV 9 min arc.
Red: SII 120 min (4x30 min subs)
Green: H-alpha 440 min (29x10+5x30)
Blue: OIII 390 min (30x10+3x30)
The top right hand butterfly wing shows a complex tracery of veins, which in most amateur images appear a black void.
Beyond the top right border of the wing is a series of blobs in H-alpha, the total effect being like an amoeba that has burst open, discharging unwanted matter. However, this blobby material may not be actually part of the nebula, as there is more of it scattered (very faintly) about the image.
Underneath the top right wing, and about 25% of the way toward 3 or 3:30 from the centre of the body, is a squashed ring structure, which on close examination seems to be made up of beads.
It is interesting to compare with the famous Hubble shot (www.apod.nasa.gov/apod/ap090910.html), and with an ESO La Silla (www.spacetelescope.org/images/heic0407b/) shot using the 3.6 metre scope. These two professional shots differ greatly from each other, perhaps in part because they use different filters.
We don't come anywhere near even the ground based ESO image for sharpness of course, but we're mostly matching them for depth. The ESO shot shows some differences in the region of the antennae, which we guess is again due to different filters. Our antennae show more in OIII, theirs more in some other warm-coloured unspecified channel, and the morphology is different.
Original image here (www.photos.smugmug.com/Category/Planetary-Nebulae/i-67WkfH6/0/O/Bug%20Nebula%20NGC%206302%20Ha%2044 0%20OIII%20390%20SII%20120%20min.jp g) has an embedded colour profile and is very slightly less compressed.
Aspen CG16M on 20" PlaneWave. Processing using GoodLook 64.
Hope you like it too.
Hubble palette, but with stars whitened. 0.55 sec arc/pixel. FOV 9 min arc.
Red: SII 120 min (4x30 min subs)
Green: H-alpha 440 min (29x10+5x30)
Blue: OIII 390 min (30x10+3x30)
The top right hand butterfly wing shows a complex tracery of veins, which in most amateur images appear a black void.
Beyond the top right border of the wing is a series of blobs in H-alpha, the total effect being like an amoeba that has burst open, discharging unwanted matter. However, this blobby material may not be actually part of the nebula, as there is more of it scattered (very faintly) about the image.
Underneath the top right wing, and about 25% of the way toward 3 or 3:30 from the centre of the body, is a squashed ring structure, which on close examination seems to be made up of beads.
It is interesting to compare with the famous Hubble shot (www.apod.nasa.gov/apod/ap090910.html), and with an ESO La Silla (www.spacetelescope.org/images/heic0407b/) shot using the 3.6 metre scope. These two professional shots differ greatly from each other, perhaps in part because they use different filters.
We don't come anywhere near even the ground based ESO image for sharpness of course, but we're mostly matching them for depth. The ESO shot shows some differences in the region of the antennae, which we guess is again due to different filters. Our antennae show more in OIII, theirs more in some other warm-coloured unspecified channel, and the morphology is different.
Original image here (www.photos.smugmug.com/Category/Planetary-Nebulae/i-67WkfH6/0/O/Bug%20Nebula%20NGC%206302%20Ha%2044 0%20OIII%20390%20SII%20120%20min.jp g) has an embedded colour profile and is very slightly less compressed.
Aspen CG16M on 20" PlaneWave. Processing using GoodLook 64.
Hope you like it too.