Bode's Galaxy (M81), The Cigar Galaxy (M82), and the Garland Galaxy (NGC 3077) gathered from my back patio in March-April, 2023. I was able to sneak this acquisition in during the few clear nights within the last couple of months using my secondary astro-rig.
You might recognize Bode's Galaxy (M81, center) from a recent post (
post 2009), and the Cigar Galaxy (M82, lower-left) from a post I made almost a year ago (
post 1681), where both of those images were acquired using my primary setup.
The Garland Galaxy (NGC 3077, lower-right) is new to me, however. The galaxy gets its name for the dwarf structure nearby the NGC 3077 galaxy itself. Either that or it gets its name from another group of stars (most in our Milky Way Galaxy) that appears -- at first glance -- as though it's about to be wrapped around NGC 3077 like a string of garland about to be wrapped around a Christmas tree. Anyway, the extra-galactic dwarf structure has been nicknamed, the "Garland." It should be noted that most of the background stars in the image (aside from the galaxies themselves) are not actually in the background at all, but rather they are quite close to us in the foreground of our own Milky Way Galaxy. The Garland, on the other hand, is not in the Milky Way; it
really is in the M81 group, near NGC 3077. What appears to be just a handful of dim stars and nebulous knots are actually some exceptionally bright stars in and around star clusters and active regions of star formation in a whole 'nother galaxy system, some 13 million light-years away.
Here's a 1:1 crop of NGC 3077 and its nearby "Garland" structure. (My little 80 mm refractor isn't able to resolve The Garland into individual stars. Anyway, The Garland is the faint area just to the right of the galaxy):
The formation of the Garland is still an area of active study; it presents a few mysteries that haven't been fully solved yet. That said, the conventional wisdom is that the Garland was formed by chaotic, tidal interactions involving a "close call" between M81 and NGC 3077 whipping past each other eons ago.
Equipment:
Explore Scientific 80ED-FCD100
Sky-Watcher EQ6-R Pro
Orion Field Flattener for Short Refractors
Off-axis guider (OAG) with guide camera
Optolong L-Pro filter
Baader Hα 3.5nm Ultra-Narrowband filter
ZWO LRGB filter set
ZWO ASI2600MM-Pro main camera
Software:
N.I.N.A.
PHD2 guiding
PixInsight with RC-Astro plugins
Integration:
Location: San Diego
Bortle class 7 (maybe 8 ) skies.
All subframes binned 1x1
L-Pro: 239×120s = 7.97 hrs
Hα: 59×600s = 9.83 hrs
R: 125×120s = 4.17 hrs
G: 63×120s = 2.10 hrs
B: 100×120s = 3.33 hrs
Total integration time: 27.4 hours.
(Here's a link to more information on The Garland:
https://articles.adsabs.harvard.edu//full/1985MNRAS.217..731K/0000731.000.html)
"A long time ago in a galaxy far, far away,..." Hold on, the M81 group isn't all that far away from us comparatively. 13 million light-years is actually pretty close in terms of galaxy cluster scales. Let me start over. "A long time ago in a galaxy that isn't really all that too terribly far away, galaxy-wise that is, ..." Hmm. 'Doesn't have the same ring to it. ... I'm just going to stop now.
Here's a crop of the image showing just M82 and M81.