Trevorw Posted March 14, 2009 Share Posted March 14, 2009 Target: NGC4372 Camera: Canon 350d modified Exposure Capture: DLSR Focus Scope: SV80ED Mount: EQ6 Pro Exposure Setting: Prime focus, ISO800 ICNR off Daylight WB Exposures: 20 x 90s 13/03/09 Seeing: Average although 90% Gibbous moon Guiding: Orion Starshoot Autoguider using PHD, although alignment was out Focus: DSLR Focus Stacking: DSS, 10 darks, 5 flats applied Processing: PS7 Info: Situated in the Musca RA: 12:25:45.4 Dec: -72:39:33 Distance from Sun: 18.9 kly Distance from Galactic Center: 23.2 kly Apparent Diameter: 18.6 arc min Brightness: 7.24 mag vis : Discovered by James Dunlop on April 30, 1826. Globular cluster NGC 4372 was discovered by James Dunlop on April 30, 1826, and cataloged as Dunlop 67. NGC 4372, a southern globular cluster of very low metallicity and very low central concentration, was chosen for a CCD photometric search for short-period binaries and SX Phe variables. We report the discovery of 19 variable stars with well-determined light curves and periods. Eight of these belong to the SX Phe class, and eight are contact binaries. All the SX Phe variables are concentrated towards the centre of the cluster and are blue stragglers, while contact binaries occupy various locations in the cluster colour-magnitude diagram. Half of the SX Phe stars pulsate in the fundamental mode, and the other half probably pulsate in the first overtone. An eclipsing variable that is either a short-period detached main-sequence binary or a cataclysmic binary is discovered Link to comment Share on other sites More sharing options...
Taff Posted March 14, 2009 Share Posted March 14, 2009 Hi Trevor'Nice write up great capture.Mark Link to comment Share on other sites More sharing options...
JCJC Posted March 14, 2009 Share Posted March 14, 2009 Trevor, great image, very detailed write up.Jordan Link to comment Share on other sites More sharing options...
Sam Posted March 14, 2009 Share Posted March 14, 2009 Excellent image Trevor - looks like a dark nebula above it too? Link to comment Share on other sites More sharing options...
Tim Posted March 14, 2009 Share Posted March 14, 2009 It's a nice cluster, but the dark cloud has caught my attention too. Where is it from, any idea? Is it attached to a bright nebula somewhere along the line?CheersTJ Link to comment Share on other sites More sharing options...
Trevorw Posted March 14, 2009 Author Share Posted March 14, 2009 The dark nebular above the cluster too the left is calledThe Dark Doodadattached is an image by Credit & Copyright: Andrey Oreshkoto show it in detail Link to comment Share on other sites More sharing options...
centroid Posted March 15, 2009 Share Posted March 15, 2009 Nice capture Trevor, and a very informative write-up to go with it.Thanks for 'posting'.I look forward to seeing those 'southern delights' again, when I get back over to WA again, later this year.Dave Link to comment Share on other sites More sharing options...
Tim Posted March 15, 2009 Share Posted March 15, 2009 ah yes, the famous Dark Doodad!! Link to comment Share on other sites More sharing options...
Trevorw Posted March 16, 2009 Author Share Posted March 16, 2009 Thanks for all the positive feedback much appreciatedCheers Link to comment Share on other sites More sharing options...
Tim Posted March 16, 2009 Share Posted March 16, 2009 Just another note to say that the way Trevor has presented his image, with the exposure details, camera setting etc is really appreciated, especially by those who are new to imaging.It would be great if we could all (I know, me too ) spend just a couple of minutes more providing that info with the pictures please. Now that SGL is the most popular astronomy site in the UK and getting busier by the day, i'm sure it would be much appreciated by the newcomers if they can see at a glance what sort of settings they will need to use, and what results they can expect.Thanks Trevor for the excellent post, looking forward to many more from you!CheersTJ Link to comment Share on other sites More sharing options...
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