Calabash Nebula
Template:Short description Template:Infobox nebula
File:QXPupLightCurve.png A near-infrared (I band) light curve for QX Puppis, plotted from AAVSO data[1] | |
| Characteristics | |
|---|---|
| Evolutionary stage | OH/IR star[2] |
| Spectral type | M10III + A[2] |
| Variable type | Mira[2] |
| Database references | |
| SIMBAD | data |
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The Calabash Nebula, also known as the Rotten Egg Nebula or by its technical name OH 231.84 +4.22, is a protoplanetary nebula (PPN) Script error: No such module "convert". long and located some Script error: No such module "convert". from Earth in the constellation Puppis. The name "Calabash Nebula" was first proposed in 1989 in an early paper on its expected nebular dynamics, based on the nebula's appearance.[3] The Calabash is almost certainly a member of the open cluster Messier 46, as it has the same distance, radial velocity, and proper motion.[4] The central star is QX Puppis, a binary composed of a very cool Mira variable and an A-type main-sequence star.
Ground-based imagery
In wide field images, the Calabash nebula is visible near the bright planetary nebula NGC 2438 in deep photographs. Although the Calabash Nebula is at the same distance as M46, NGC 2438 is a larger object in the foreground.
Notes
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- <templatestyles src="Citation/styles.css"/>^ Radius = distance × sin(angular size / 2) = 5 kly * sin(1Template:Prime / 2) = 0.7 ly
- <templatestyles src="Citation/styles.css"/>^ 9.47 apparent magnitude - 5 * (log10(1,500 pc distance) - 1) = -1.4 absolute magnitude
References
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Sources
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External links
- PIA04228: Rotten Egg Nebula, NASA Planetary Photojournal
- The Rotten Egg Planetary Nebula, APOD 1999 November 1
- The Making of the Rotten Egg Nebula, APOD 2001 September 3
- Calabash Nebula at Constellation Guide
- Calabash Nebula imaged and interpreted by Bo Reipurth at the European Southern Observatory in 1987
