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SH2 104,LBN 195,DWB 18, GM 1-27 (Cygnus)
M101 (Ursa Major)
IC5076 (vdB 137),vdB 138,LDN 958,GN 20.57.4,LDN 955 (Cygnus)
IC5146 ,vdB 147,CGN 185 (Cygnus)B
 NGC 918 ,MBM8,MBM7 (Aries)
  PGCC Clouds,NGC 7223 (Lacerta).jpg - Plank Galactic Cold Clumps , NGC 7223,UGC 11927  (Lacerta) * October-November 2019 * CFF 135 mm telescope (f/6.7, 930mm) * ASA DDM 85 mount * G3 16200 EC Moravian CCD* Baader LRGB filter set* L:507 minutes R: 411 m G: 337 m B:431m * Planck satellite mission.The Planck Catalogue of Galactic Cold Clumps (PGCC) is a list of 13188 Galactic sources and 54 sources located in the Small and Large Magellanic Clouds. The sources have been identified in Planck data as sources colder than their environment and following the spatial distribution of the main molecular cloud complexes. The median temperature of PGCC sources lies between 13 and 14.5 K.It´s the result of combinning the Planck-HFI and IRAS maps to perform an all-sky detection of the cold submillimetre Galactic sources over the whole sky. The main feature of this image field is the series of molecular clouds from upper left to bottom right . These clouds are cataloged in the Planck Catalog of Galactic Cold Clumps (PGCC), but they are not in any of the well known Astronomical catalogs. Also in the field is a significant number of background galaxies - some of them are visible through the molecular clouds. One of these galaxies is from the NGC catalog (NGC 7223). Many of these  background galaxies are members of galaxy groups.  Credits commentaries: Jim Thommes, Antonio F. Sanchez.  
 
 
 
 
 

Plank Galactic Cold Clumps , NGC 7223,UGC 11927 (Lacerta) * October-November 2019 * CFF 135 mm telescope (f/6.7, 930mm) * ASA DDM 85 mount * G3 16200 EC Moravian CCD* Baader LRGB filter set* L:507 minutes R: 411 m G: 337 m B:431m * Planck satellite mission. The Planck Catalogue of Galactic Cold Clumps (PGCC) is a list of 13188 Galactic sources and 54 sources located in the Small and Large Magellanic Clouds. The sources have been identified in Planck data as sources colder than their environment and following the spatial distribution of the main molecular cloud complexes. The median temperature of PGCC sources lies between 13 and 14.5 K. It´s the result of combinning the Planck-HFI and IRAS maps to perform an all-sky detection of the cold submillimetre Galactic sources over the whole sky. The main feature of this image field is the series of molecular clouds from upper left to bottom right . These clouds are cataloged in the Planck Catalog of Galactic Cold Clumps (PGCC), but they are not in any of the well known Astronomical catalogs. Also in the field is a significant number of background galaxies - some of them are visible through the molecular clouds. One of these galaxies is from the NGC catalog (NGC 7223). Many of these background galaxies are members of galaxy groups. Credits commentaries: Jim Thommes, Antonio F. Sanchez. Download Imagen original
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