Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  23 Cep  ·  23 eps Cep  ·  B369  ·  HD210922  ·  HD211070  ·  HD211336  ·  HD211430  ·  HD211472  ·  HD211489  ·  HD211554  ·  HD211643  ·  HD211774  ·  HD211820  ·  HD211982  ·  HD212043  ·  HD212106  ·  HD212183  ·  HD212200  ·  HD212312  ·  HD212455  ·  HD212533  ·  HD235749  ·  HD235775  ·  HD235783  ·  HD235805  ·  HD235809  ·  HD235813  ·  HD239928  ·  LBN 471  ·  LBN 473  ·  And 8 more.
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SH2-132 in HOO, Miguel A.
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SH2-132 in HOO

Acquisition type: Electronically-Assisted Astronomy (EAA, e.g. based on a live video feed)
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SH2-132 in HOO, Miguel A.
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SH2-132 in HOO

Acquisition type: Electronically-Assisted Astronomy (EAA, e.g. based on a live video feed)

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Description

First night running 3 widefield scopes.

Object for the night was, the Lion Nebula, Sh2-132 is a large emission nebula visible in the constellation Cepheus. It is located on the southern edge of the constellation, a short distance from the boundary with the Lizard, along the plane of the Milky Way; the best period for its observation in the evening sky falls between July and December and is greatly facilitated for observers located in the northern hemisphere regions of Earth. Sh2-132 is located at a distance of nearly 3200 parsecs (almost 10400 light-years), thus placing it within the Perseus Arm, in the region of Cepheus OB1, a large and bright OB association. The stars responsible for the ionization of its gas are very hot and massive; in particular, two Wolf-Rayet stars have been identified, known as HD 211564 and HD 211853 (the latter also having the abbreviation WR 153), as well as a spectral class O8.5V star and about ten B-class stars. Around the O-class star and one of the Wolf-Rayet stars extends a bubble clearly visible in the radio wave band, identified as Shell B, probably originating from the stellar wind of the two massive stars. A similar but smaller structure, Shell A, hosts a K-class star near its center. Chain star formation processes are believed to have taken place in the nebula in the past; currently, these processes appear to be suspended since there is no evidence of recent activity. Nine sources of infrared radiation and a maser with H2O emissions have been detected in the direction of the nebula.

(Source: Wikipedia)

I imaged this object in early November. One night I was used 3 rigs., a first for me. The setup went really well. Took about 35 minutes to get all 3 imaging the object. Seeing was not the greatest.

Processing this object to get accurate colors in Hydrogen Alpha and Oxygen was a little challenging.

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