Celestial hemisphere:  Southern  ·  Constellation: Scorpius (Sco)  ·  Contains:  B257  ·  NGC 6334  ·  Sh2-8
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NGC 6334 A Star-Burst HII Region in LSHO, Alex Woronow
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NGC 6334 A Star-Burst HII Region in LSHO

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NGC 6334 A Star-Burst HII Region in LSHO, Alex Woronow
Powered byPixInsight

NGC 6334 A Star-Burst HII Region in LSHO

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Description

NGC 6334 A Star-Burst HII Region in LSHO

OTA: TAO 150 (f/7.3)

Camera: FLI - ML16200 (1.13 arcseconds/pixel)

Observatory: Deep Sky West, Chile

EXPOSURES:

H: 21 x1800 sec.

S: 11 x 1800

O: 15 x 1800

L: 19 x 600

Total exposure ~28 hours

Image Width: ~1.4 deg

Processed by Alex Woronow (2020) using PixInsight, Skylum, Topaz, SWT

NGC 6334 is a souther-sky “Star-Burst” cluster in our own galaxy. It lies about 5,500 light-years from us in the direction of the galactic center and nearly in the galactic plane. The cluster itself inhabits the redish cloud in the upper right of this image. The term “star-birst region” denotes a region where exceptional rapid star formation has arisen. In this case the triggering event for the star-burst may have been the collision between two giant molecular clouds (Fukui, et al. 2018).

The stars young and massive in NGC 6334 emit winds that rake the HII parent cloud, sculpting the dust and gas into streaks, loops, and bubbles. However, Hua-bai Li and colleagues (2015) found relationships between the magnetic fields in NGC 6334 and filiment structures in the cloud strures, suggesting that the cloud may be too young to have yet been effected by the winds from the young stars, which should dominate. Or, maybe as Wade (2014) suggests, the magnetic fields of the O stars themselves may direct the paths of their stellar winds.

The cloud stands apart from other clouds hosting star-burst activities in that it has the most intense emissions from ammonia known for any such cloud (Kuiper, et al. 1995). Taken together, the magnetic-lines controling structres and the presence o ammonial, The cloud and star-burst ages appear to be quite young, perhaps only about a million years old.

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