Melotte 15 was my primary objective, but given my wide field and camera I get the most of the rest.  I have provided a mouse-over sub frame of the central part of the larger image.  I have always admired the dust/gas cloud structures that this cluster of young intense stars has sculpted.  It sits right in the middle of IC 1805, common name The Heart.  It is very likely that the whole of IC 1895 is a local bubble cleared out by the intense UV irradiation from these stars.  But the structures that appear closest to the cluster are the most dramatic.  I deduce they are closest, but instead, we may be looking at the tip of a cloud column that falls away from us, from our perspective with the cluster superimposed.  Who knows?  But there are other clues, I think.  The spiral and bifurcating column seems illuminated the very brightest when compared to the perimeter "Heart", which seems to glow mostly in excited hydrogen with a bit of blue component evident in some areas inside the perimeter.  The dramatic columns appear embedded within a diffuse reflection component that seems to include some of the stars.  Reflection nebulae usually are more closely associated with their source of illumination, something that hydrogen excitation does not suffer so much from.  I will go with the theory that we are looking down at the top of a dust/gas cloud that closely approaches near or through the cluster and extends beyond, visually appearing to the lower left.  I say this because the arrow shaped shadowed portion of this cloud belies its position above most of the bright stars (hence the reason it is not illuminated).  As such, the whole column may actually continue, broken up, all the way to the dark nebulae at roughly 7 o'clock, which show us their shaded, unilluminated sides in rather dramatic fashion.

I have done a fair amount of star reduction of the image to highlight the outer reaches of the Heart.  However, I tried to leave a light touch with the bright stars in Melotte 15, since I wanted to leave the impression that there is obvious impact of the brightness of these stars on the formation of the structures.  Its hard for me to make sense visually of reflection nebulae being brighter than the stars that illuminate them!  

It is not surprising that this whole area is filled with young stellar objects.  In fact many of the very brightest stars seen here are listed as YSO.  This information I gathered from Simbad.  I should be careful when I describe an area as a hotbed of star formation because what is reported by Simbad is often findings from astonomers having concentrated their efforts in a particular area.  You see these astronomer-studied hot spots often, with a telltale signature when the area of hot activity is all concentrated in the shape of a square, or perfect circle.  So just because other areas displayed by Aladin may not list a lot of activity, it may actually be due to the fact that the professionals have yet to turn their gear on those areas yet and/or just not reported it yet.

For QHY 268C users, I chose extended deep well mode #3, and used a gain of 0, offset 8.  All hoping to not saturate bright stars.  ~90,000 e-, if you believe the numbers...