Celestial hemisphere:  Southern  ·  Constellation: Carina (Car)  ·  Contains:  HD96265  ·  HD96309  ·  HD96548
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RCW58, John Dziuba
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RCW58

Getting plate-solving status, please wait...
RCW58, John Dziuba
Powered byPixInsight

RCW58

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Description

RCW58 is an E type nebula, formed by a bubble of ejecta around the massive Wolf Rayet star WR40.  When viewed in two dimensions, it appears as a ring.  In these type of nebula, it is common to see the outer most edge O3 emission leading the Ha emission.  This is due to the shock wave from the Wolf Rayet bubble expanding into the surrounding envelope. 

Although the shape and mechanism (central star ejecta) responsible for the formation of the bubble is similar to that of a planetary nebula,  the nature of the central star is completely different.  Wolf Rayet stars are immense, short lived, and extremely hot stars that usually end their short lives in a supernova.  Planetary nebula have much smaller degenerate stars at their centers, usually a white dwarf.  Both types eject material from their atmospheres, causing the ionized bubble to form.

This was an exceedingly difficult image to process, and this explains why there are so few images of this object on Astrobin.  The signal is weak and the star field is dense.  My goal was to separate and amplify the extremely faint background Ha signal and the very faint O3 signal from the noise floor.  I collected 42hrs of data which is more than my usual in order to resolve these faint features.

Hope you like it.
CS

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RCW58, John Dziuba