Celestial hemisphere:  Southern  ·  Constellation: Vela (Vel)  ·  Contains:  NGC 2626  ·  NGC 2671  ·  The star d Vel  ·  The star e Vel
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The Vela Molecular Ridge (RCW27, RCW32, and RCW33), Charles Bracken
The Vela Molecular Ridge (RCW27, RCW32, and RCW33)
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The Vela Molecular Ridge (RCW27, RCW32, and RCW33)

Getting plate-solving status, please wait...
The Vela Molecular Ridge (RCW27, RCW32, and RCW33), Charles Bracken
The Vela Molecular Ridge (RCW27, RCW32, and RCW33)
Powered byPixInsight

The Vela Molecular Ridge (RCW27, RCW32, and RCW33)

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Description

The Vela Molecular Ridge is a series of HII regions that run along the northern edge of the Vela Supernova Remnant. This eight-panel mosaic taken from Chile captures nearly five degrees vertically. The image here is 1/4th the full-size image, which is 382 megapixels in size! This image was a collaboration over two months with Charles Pevsner, Max Whitby, and Raymond Protière.

RCW27 is at upper left, RCW32 in the middle, and RCW33 at bottom right. Part of the Vela SNR can be seen at upper right. The small reflection nebula embedded in RCW27 is NGC2626. The bright spot at lower-right is Kohoutek 2-15, an HII region miscategorized as a planetary nebula. There are several real planetary nebulae visible as well: Wray 16-23 is at upper left, and Wray 16-32 is at bottom left. (There are others, but they are nearly stellar in size.

The slightly odd magenta and red hues on the right are due to the unusual mixture of ionized gases in the Vela SNR. You don’t normally get SII signal without H-alpha like that outside of SNRs or planetary nebulae.

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    The Vela Molecular Ridge (RCW27, RCW32, and RCW33), Charles Bracken
    Original
  • Final
    The Vela Molecular Ridge (RCW27, RCW32, and RCW33), Charles Bracken
    B

B

Description: Revision: we felt it looked better rotated 180 degrees, and a slight contrast enhancement curve was also applied.

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The Vela Molecular Ridge (RCW27, RCW32, and RCW33), Charles Bracken