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Contains:  The star γ2Vel, The star γ1Vel
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Vela SNR - LAmbda Velorum region

Technical card

Resolution: 2984x2269

Dates:Feb. 2, 2019

Frames: 26x1800"

Integration: 13.0 hours

Avg. Moon age: 27.41 days

Avg. Moon phase: 5.01%

Astrometry.net job: 2503640

RA center: 123.557 degrees

DEC center: -46.435 degrees

Pixel scale: 3.276 arcsec/pixel

Orientation: 182.895 degrees

Field radius: 1.706 degrees

Locations: Burwood, Melbourne, Victoria, Australia

Data source: Backyard

Description

A wave of Ionised Oxygen (O3) streaks across the background clouds of Hydrogen (Ha). It is believed to result from a powerful explosion of a star some 11,000 -12,000 years ago. The shock waves shown in the image as blue from oxygen emission and red from hydrogen emission have been expanding ever since.

The huge star at the top left is Gamma Velorum, a quadruple star system in the constellation Vela. At a combined magnitude +1.7, it is one of the brightest stars in the night sky, and contains by far the closest and brightest Wolf-Rayet star. It has the traditional Arab name Suhail al Muhlif.
(wiki)

The open cluster at the centre is Collinder 173. :)

Image & processing inspired by Marco Lorenzi.

SV70t Refractor on TAK NJP mount - QSI 683 wsg8 camera.
Ha 240mins, O3 540mins, RGB 30mins ea.

Taken over 3 nights from from Burwood, Suburban Melbourne.:D

Comments

Author

Andys_Astropix
Andys Astro
License: None (All rights reserved)
3908
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Vela SNR - LAmbda Velorum region, 





    
        

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