NGC 6164, NGC 6165 and the Blue Doily Nebula

 

 

 

 

Click on the image for a full resolution version

       See this image also on Instagram

 

 

 

This image shows way more than strictly the red emission nebulas NGC 6164 and 6165. NGC 6164 is the bright bar located in the lower left (Northeastern) part of the central red nebulosity. NGC 6165 is the bright bar located in the upper right (Southwestern) part of it. This nebula is the result of the mass ejection by an infrequent star type, O6.5f (only five such stars are known, three in our own galaxy and two in the Small Magellanic Cloud). This nebulosity is the result of a two-step fierce mass ejection from the central star. HD 148937 is a massive, very hot, spectroscopic binary star, with a combined mass about 40 times that of our Sun. This kind of stars live fast and last short. Its age has been calculated in about four million years and still has about two to three million years to go. At its end, it will most probably explode as supernova. Stars of this kind (O6.5f) burn hydrogen through the CNO cycle. This cycle is responsible for the notably higher than usual concentration of nitrogen in the nebula. According to one theory, the complex structure that is seen in the inner nebula (very notably the bluish wisps and a cone, both bright in the [OIII] line) can be due to the stars’ rotation in addition to strong magnetic fields that can be sculpting the whole gas nebula. Several so called “cometary knots” can be spotted in the brightest bars and are probably due to the impact of the stellar wind on slower, denser shells of gas.

The external bluish nebulosity is much fainter and very rich in [OIII]. This bubble-like nebulosity (of which I haven’t found any existing specific name) is the result of an earlier mass ejection by the same star. It already interacts with the surrounding hydrogen-rich gas in its region.

Object

Name(s): NGC 6164/NGC 6165

Type: Emission Nebula

RA:  16h 33m 52s

Dec: -48º 06’ 41”

Constellation: Ara

Size (arcmin): 21×13

Magnitude: +11

Distance: 4,200 ly

Image

Date: 2023-03-22 to 2023-04-01

Location: Obstech, Río Hurtado, Chile

Size (arcmin): 33×26 arcmin

Telescope: 24” f/6.5 Reflector

Camera: QHY 461 (11760x8896pix)

Guiding: off-axis guider

Total exposure: 29 hours (Ha: 10h; [OIII]: 16h; RGB: 3h)

Processing: CCDStack, PixInsight (one process) and Photoshop CC 2023

error: Content is protected !!