MAPOW Nr 7: A false color Flaming Star Nebula

Auriga is really a treasure box of bright astronomical objects: star clusters, bright nebulas and dark nebulas. Among them all, IC 405, the Flaming Star Nebula, is one of the most photographed objects.

This image is an unusual Hα–SII bicolor composition in false color. The Hα and SII emission lines both lie in deep red, so it is impossible to render colour differences in a realistic way: the only option is a false color composition.

In this image hydrogen emission has the usual pinkish color due to the Hα and Hβ emission lines. As said before, the SII emission line lies in deep red but, on Earth, crystalline sulfur has yellow hues, so my goal was to render the SII in yellow.

To accomplish my goal I used the PixelMath tool in PixInsight. The composition formula was:

R channel:  Hα
G channel:  SII
B channel:  0.25*Hα - 0.75*SII

The B channel formula is very simple: the 0.25*Hα accounts for the Hβ emission, giving the hydrogen emission its usual pinkish color; subtracting the SII emission shifts the color hue of the sulfur-rich zones toward yellow. The 0.75 factor is an arbitrary value chosen to render the wanted color.

All the image processing was done in PixInsight.

The Flaming Star Nebula IC 405 in false color

IC 405, The Flaming Star Nebula

Date and locationCastenedolo — October 31, November 1st 2015
SensorSBIG ST2000XV
TelescopeWilliam Optics FLT 100 with Type III focal reducer
Mount10Micron GM1000 HPS
ExposureHα: 31x600s
SII: 26x900s
AuthorEdoardo Luca Radice
NotesSingle unguided exposures with the 10Micron HPS system — Processing: PixInsight 1.8