Celestial hemisphere:  Northern  ·  Constellation: Hercules (Her)
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LBN 105 (AKA Sh2-73), George Simon
LBN 105 (AKA Sh2-73)
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LBN 105 (AKA Sh2-73)

Getting plate-solving status, please wait...
LBN 105 (AKA Sh2-73), George Simon
LBN 105 (AKA Sh2-73)
Powered byPixInsight

LBN 105 (AKA Sh2-73)

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Description

Almost every published image of LBN 105 that I examined in preparation for publishing my own image includes a commentary relating the same facts about this object. However, since LBN 105 is rather infrequently imaged, many of you might not be aware of these facts. So, at the risk of being repetitive, I, too, am going to relate the same basic facts.

LBN 105 was originally characterized as an emission nebula. Accordingly, Stewart Sharpless included it as the 73rd entry in the second edition of his catalogue of HII regions. More recently, it has been discovered that LBN 105 is not an HII region, but is, in fact, a molecular cloud, with no signs of star formation occurring within it. Located at a distance of about 400 light years from Earth, and at a galactic latitude of about 45º, LBN 105 sits considerably above the Milky Way's disk and reflects the integrated light of the entire galaxy. LBN 105 is thus a classic instance of IFN. Its peculiar hairpin shape is apparently pretty typical of the shape of local molecular clouds.

As one might imagine, given the dimness that characterizes most instances of IFN, this image was a monumental pain to process. I could have made things easier on myself by collecting at least twice as much data, but we are entering the season here in South Carolina when clear nights are hard to come by, due to lingering cloud debris from afternoon and evening pop-up thunderstorms. So, I went with what I had and battled with the noise attending upon the hard stretch of the data that I had to do to reveal LBN 105 and at least some of the dimmer nebulosity in which it is embedded.

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LBN 105 (AKA Sh2-73), George Simon

In these public groups

Cloudy Nights