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NGC 4151 (Eye of Sauron),NGC 4156 (Canes Venatici)
NGC 5934,5935,5943,5945,5947 (Bootes)
LDN 810,SH2-92,Reflection nebula GN 19.43.3.01, YSO CB205YC1 (Vulpecula-Cygnus)
vdB 136,LBN 312 (Cygnus)
LBN 331,DWB 177,DWB 178,DWB 179, V1488 Cyg (Cygnus)
  LBN 248, HH425 (Cygnus).jpg - LBN 248,Herbig-Haro 425 (Cygnus) * August 2015 * ASA N12 astrograph (f/3.6, 1078mm) * DDM85 ASA mount * FLI ML8300 * LRB Optec filter set * L:410m R:170m G:160m B:200m * Unguided * Herbig–Haro (HH) objects are small patches of nebulosity associated with newly born stars, and are formed when narrow jets of gas ejected by young stars collide with clouds of gas and dust nearby at speeds of several hundred kilometres per second. Herbig–Haro objects are ubiquitous in star-forming regions, and several are often seen around a single star, aligned with its rotational axis.HH objects are transient phenomena, lasting not more than a few thousand years. They can evolve visibly over quite short astronomical timescales as they move rapidly away from their parent star into the gas clouds of interstellar space (the interstellar medium or ISM). Hubble Space Telescope observations have revealed the complex evolution of HH objects over the period of a few years, as parts of the nebula fade while others brighten as they collide with clumpy material of the interstellar medium.The objects were first observed in the late 19th century by Sherburne Wesley Burnham, but were not recognised as being a distinct type of emission nebula until the 1940s. The first astronomers to study them in detail were George Herbig and Guillermo Haro, after whom they have been named. Herbig and Haro were working independently on studies of star formation when they first analysed the objects, and recognised that they were a by-product of the star formation process.LBN 248 is a  very interesting and strange reflection nebula surrounding the low part of the photograph. This area is rarely  imaged. Thanks to Mr. Sakib Rasool for suggesting this target. .Information credits:  Reipurth B. (1999). "A General Catalogue of Herbig–Haro Objects,".Wikipedia.  
NS2,LDN 1299 (Cassiopeia)
TGU H774 P19,vdB 2,LBN 590,V V510 Cas (Cassiopeia)
DG 41 (GN 04.32.08, Magakian 77), HH 434,435,436,LDN 1536 (Taurus)
BSF32 (Perseus)
NGC 4449 (Canes Venatici)

LBN 248,Herbig-Haro 425 (Cygnus) * August 2015 * ASA N12 astrograph (f/3.6, 1078mm) * DDM85 ASA mount * FLI ML8300 * LRB Optec filter set * L:410m R:170m G:160m B:200m * Unguided * Herbig–Haro (HH) objects are small patches of nebulosity associated with newly born stars, and are formed when narrow jets of gas ejected by young stars collide with clouds of gas and dust nearby at speeds of several hundred kilometres per second. Herbig–Haro objects are ubiquitous in star-forming regions, and several are often seen around a single star, aligned with its rotational axis. HH objects are transient phenomena, lasting not more than a few thousand years. They can evolve visibly over quite short astronomical timescales as they move rapidly away from their parent star into the gas clouds of interstellar space (the interstellar medium or ISM). Hubble Space Telescope observations have revealed the complex evolution of HH objects over the period of a few years, as parts of the nebula fade while others brighten as they collide with clumpy material of the interstellar medium. The objects were first observed in the late 19th century by Sherburne Wesley Burnham, but were not recognised as being a distinct type of emission nebula until the 1940s. The first astronomers to study them in detail were George Herbig and Guillermo Haro, after whom they have been named. Herbig and Haro were working independently on studies of star formation when they first analysed the objects, and recognised that they were a by-product of the star formation process. LBN 248 is a very interesting and strange reflection nebula surrounding the low part of the photograph. This area is rarely imaged. Thanks to Mr. Sakib Rasool for suggesting this target. . Information credits: Reipurth B. (1999). "A General Catalogue of Herbig–Haro Objects,".Wikipedia. Download Imagen original
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