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NGC  2014 & 2020 in the Large Magellanic Cloud, Alex Woronow
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NGC 2014 & 2020 in the Large Magellanic Cloud

Getting plate-solving status, please wait...
NGC  2014 & 2020 in the Large Magellanic Cloud, Alex Woronow
Powered byPixInsight

NGC 2014 & 2020 in the Large Magellanic Cloud

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NGC  2014 & 2020 in the Large Magellanic Cloud

OTA:……………….CHI-1: CDK24 f/65
Camera:………….FLI PL9000
Observatory:…. Telescope Live, Chile

EXPOSURES:                
…H: 16 x 600        
…S: 17 x 600        
…O: 20 x 600        
Total exposure    9.2 hours

Image Width: 30 arc-minutes
Processed by Alex Woronow (2022) using PixInsight, Topaz, 3DLut, SWT

This image of NGC 2014, a violent star-forming area in the Large Magellanic Cloud, started from a true-color mapping of the narrowband filters. The blue cloud to the lower left is NGC 2020.

The blue parts of NGC 2014 and NGC 2020 are not, as one might expect, a reflection nebula, but ionized oxygen. (The OIII narrowband filters would not pick up much of a blue reflection nebula, except in the spectral continuum contribution to the image.) The loops and streamers in NGC 2014 arise from the violent star births and deaths it hosts and facilitates. Many of those young blue stars can be seen near the center of the image.

Most interestingly, perhaps, is that NGC 2020, the blue ring, was created by a single massive Wolf-Rayet star (about 200 thousand times brighter than our sun, throwing off a succession of outer envelopes of material. That WR star can be seen inside the ring of blue gas.

The image posted here is downsample almost 2::1. Image B is a patch at full resolution.

Alex

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  • Final
    NGC  2014 & 2020 in the Large Magellanic Cloud, Alex Woronow
    Original
  • NGC  2014 & 2020 in the Large Magellanic Cloud, Alex Woronow
    B

B

Title: Full Resolution Patch

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NGC  2014 & 2020 in the Large Magellanic Cloud, Alex Woronow