Processing: Data Collection -  N.I.N.A. Sequencer (as FITs).  Sub-frame calibration - Pixinsight (WBPP). Sub-frame  registration and integration (Average combine -  Linear clipping) - PixInsight (WBPP).  2x Drizzle of Lum stack - PixInsight (WBPP).  Noise reduction - NoiseXTerminator - PixInsight. Non-linear stretching, normalization and gradient removal - PixInsight. Photometric RGB calibration (SPCC) - PixInsight. Deconvolution of Lum, Emission Line, and RGB combine - BlurXTerminator. Generation of starless nebulosity Lum and combined RGB images for later processing - Star XTerminator.  Curves, Levels, RGB combine - PixInsight.  RGB starless and Lum starless  combine (for LRGB starless) - PixInsight.  LRGB stars screened to LRGB starless - Pixinsight.  Final finishing, crop, and resample  - Affinity Photo.   Annotation - PixInsight, Aladin (Simbad), and Affinity Photo. This image is an  LRGB starless composition - with LRGB stars added.  Image processed at 12496x8352 resolution. Final Image size is approximately  7196x4860.

North is down and slightly to the left in this image  (10 degree rotation - equatorial coordinates).  This image shows  the high galactic latitude Cirrus (IFN) of the LBN 629 region. This places these clouds well above the plane of the Milky Way disk. These clouds are not particularly illuminated by single stars, but instead illuminated by the bulk of the Milky Way stars close to the galactic disk.   LBN 629's galactic coordinates are roughly  126 longitude, 32 degrees latitude.  This places it a little further away from the galactic center than that of the sun and on the galaxy's north pole side. 

There are also cold clouds (called cold clumps and identified in the Planck Galactic Cold Clump Catalog) in this image. These cold clouds are noted for their low temperatures - lower than their surrounding space. They are not seen in optical wavelengths - they are observed and measured in radio wavelengths. However, they are sometimes coincident with optical wavelength structures. They are of interest since they can be precursors in the evolution of star forming regions. 

These objects and some of the brighter stars are identified in the annotated image.   Horizontal Full FOV is approximately 2.47 degrees. Full size image scale is about 1.24 arcsec/pix.