Planetary nebulae research 3

Ghost of Jupiter, NGC 3242

NGC 3242 is planetary neblua in constellation the Hydra. Image of the nebula is at the bottom of the photo. The spectrum of the nebula and stars are projected to up left from the image. Spectrum of the nebula is very strong at wavelenght 656.3nm (H-alpha) and 501nm (OIII). The spectrum is dim at infrared wavelenghts that includes 672nm (SII). Ultraviolet part of the spectrum is not visible because the atmosphere strongly absorbs ultraviolet radiation.

Telescope: ITelescopes Telescope-17 0,43m (17inch), f/6.8 (Located to Australia)

Camera: FLI PL4710 - Non Anti Blooming Gate 0.92 Arc secs/pixels

Exposure: 3 * 180s
Date: 03 Feb. 2018

Blue Snowball Nebula, NGC 7662

Hydrogen alfa	Ultraviolet

Infrared	Color

	Color 2

NGC 7662 is planetary nebula in the constellation Andromeda. The central star is visible in both infrared and ultraviolet images. The nebula resemble Ring nebula that is seen slightly sideways. The nebula has ring and central star in the center of it. The nebula has also relative bright halo around it. Telescope: ITelescopes Telescope-11 0,51m (20inch), f/6.8, f/4.5 focal reducer (Located to New Mexico USA) Camera: FLI ProLine PL11002M CCD Camera, Anti Blooming Gate, 0.81 Arc secs/pixels Filter: Infrared (806nm, Bandwidth 149nm), Ha (656.28nm), Ultraviolet (365nm, Bandwidth: 66nm) Exposure: 3 * 300s Ha, 3 * 300s I, 3 * 600s U Date: 25-27 Aug. 2018

Eskimo Nebula, NGC 2392

Hydrogen alfa	Ultraviolet

Infrared	Color

NGC 2392 is planetary nebula in the constellation Gemini. The central star is visible in all images.´The lower part of the nebula is much brighter than other outer parts of the nebula. The nebula has also lots of different structures. Telescope: ITelescopes Telescope-11 0,51m (20inch), f/6.8, f/4.5 focal reducer (Located to New Mexico USA) Camera: FLI ProLine PL11002M CCD Camera, Anti Blooming Gate, 0.81 Arc secs/pixels Filter: Infrared (806nm, Bandwidth 149nm), Ha (656.28nm), Ultraviolet (365nm, Bandwidth: 66nm) Exposure: 3 * 300s Ha, 3 * 300s I, 3 * 600s U Date: 17 Feb. 2019 Ha, 22 Mar. 2019 I, 15 Apr. 2019 U.