Placidus
19-05-2018, 01:19 PM
There are at least two galaxies that show wonderful intricate detail in H-alpha: NGC 300, and Barnard's Galaxy, an irregular dwarf in Sagittarius.
We photographed Barnard's Galaxy in 13 hours of H-alpha back in 2012, but there was considerable moon about.
Here, we've had another go at new moon. Even though we've only got 9.5 hours of H-alpha, it was much better.
Barnard's Galaxy is of pretty low surface brightness (14.4 mag/sq arcmin) even in full spectrum, so it is exceeding faint in H-alpha alone.
[Did someone say faint? This sounds like a job for ... superduck!]
Because it is so faint, we've had to brighten the image approximately 20,000 times over a raw half-hour sub. Consequently the fainter stars will look a bit gritty and the background blotchy. Guiding was also ratty due to intermittent cloud and paucity of good guide stars.
Despite these caveats, we've managed to bring out some pleasingly sharp detail in the hollow shells, intricate stringy knots, and even the odd intriguing horseshoe in the brighter patches of H-alpha nebulosity.
Here it is in H-alpha only. (Here is 9.5 hours in H-alpha only.)
We've added 2 hrs per channel RGB to guide the eye and give a feel for the whole galaxy.
Full size HaRGB image here (https://photos.smugmug.com/Category/Astrophotography-at-Placidus/i-VkFkstk/0/a31bbda0/O/Barnard%27s%20Galaxy%202018%20Ha%20 9p5%20RGB%202hrs%20each.jpg)
Toward the top of the galaxy, you will notice large swathes of bright blue star formation with remarkably little H-alpha. Presumably star formation in these regions is largely complete.
It is fun to compare the H-alpha tangles with the Answer in the Back of the Book (https://www.eso.org/public/images/eso0938a/), from the 2.2 metre ESO scope at La Silla.
Aspen CG16M on 20 inch PlaneWave. 0.55 sec arc per pixel. South probably up.
Very best,
Mike and Trish
We photographed Barnard's Galaxy in 13 hours of H-alpha back in 2012, but there was considerable moon about.
Here, we've had another go at new moon. Even though we've only got 9.5 hours of H-alpha, it was much better.
Barnard's Galaxy is of pretty low surface brightness (14.4 mag/sq arcmin) even in full spectrum, so it is exceeding faint in H-alpha alone.
[Did someone say faint? This sounds like a job for ... superduck!]
Because it is so faint, we've had to brighten the image approximately 20,000 times over a raw half-hour sub. Consequently the fainter stars will look a bit gritty and the background blotchy. Guiding was also ratty due to intermittent cloud and paucity of good guide stars.
Despite these caveats, we've managed to bring out some pleasingly sharp detail in the hollow shells, intricate stringy knots, and even the odd intriguing horseshoe in the brighter patches of H-alpha nebulosity.
Here it is in H-alpha only. (Here is 9.5 hours in H-alpha only.)
We've added 2 hrs per channel RGB to guide the eye and give a feel for the whole galaxy.
Full size HaRGB image here (https://photos.smugmug.com/Category/Astrophotography-at-Placidus/i-VkFkstk/0/a31bbda0/O/Barnard%27s%20Galaxy%202018%20Ha%20 9p5%20RGB%202hrs%20each.jpg)
Toward the top of the galaxy, you will notice large swathes of bright blue star formation with remarkably little H-alpha. Presumably star formation in these regions is largely complete.
It is fun to compare the H-alpha tangles with the Answer in the Back of the Book (https://www.eso.org/public/images/eso0938a/), from the 2.2 metre ESO scope at La Silla.
Aspen CG16M on 20 inch PlaneWave. 0.55 sec arc per pixel. South probably up.
Very best,
Mike and Trish