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Approaching Sharpless 264

Technical card

Imaging telescope or lens:Takahashi FSQ Fluorite

Imaging camera:FLI PL16803

Mount:Paramount ME

Software:MaximDL 5

Filter:Astrodon 5nm Halpha

Resolution: 4000x3289

Dates:April 5, 2019

Frames: 108x1800"

Integration: 54.0 hours

Avg. Moon age: 0.12 days

Avg. Moon phase: 0.02%

Astrometry.net job: 2626710

Data source: Own remote observatory

Remote source: Non-commercial independent facility

Description

Sharpless 264, also known as the Lambda Orionis Ring, is a molecular cloud and H II region, which can be seen in the northern region of the Orion Molecular Cloud Complex (OMCC), in the constellation of Orion. The OMCC is one of the best-known star formation regions and the closest sector of the Milky Way to our Solar System where high-mass stars are born. The nebula is named after its main star, λ Orionis, a blue giant responsible for the ionization of the surrounding material. It is also sometimes called the Angelfish Nebula due to its resemblance as to its lighter areas (pink to peach colour) to an angelfish. In the infrared its ionized boundaries are that which appears, instead. - source: Wikipedia

This is another in a series of starless interpretations in deep hydrogen alpha light using the starnet++ software. The image represents 18 individual mosaic tiles. North is to the right in this orientation.

Comments

Author

dvj
John Gleason
License: None (All rights reserved)
3084
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Histogram

Approaching Sharpless 264, 





    
        

            John Gleason