NGC 3372 (Car), Eta Carinae-complex
Click on the image for a larger version
Date/Site: |
30. and 31. January 2014, Astrofarm at the Hacienda los Andes, Chile |
Exposure/
Filter |
LRGB: each channel 6 x 900 seconds (-20°C) |
Camera: |
SBIG STL11000 with Astronomik type II-filters |
Optics/
Instrument: |
Astro-Physics 175mm f/8 StarFire EDF triplet refractor with flattener on AP1200 GTO |
|
Guiding: Lodestar attached to a 61mm-finder,
focusing: Robofocus and FocusMax,
image acquisition: CCD-Commander and MaximDL 5,
calibration and processing: PixInsight 1.8 |
As with the Tarantula nebula I like the LRGB-image best.
The HαLRGB-version seems to me too much dominated by red. Here too the strong O3-signal, which is prominent visually, is missing. So I have to make O3 next time :-)
Eta Carinae-complex (Carina), HαLRGB-version
Click on the image for a larger version
Date/Site: |
30. and 31. January 2014, Astrofarm at the Hacienda los Andes, Chile |
Exposure/
Filter |
LRGB: each channel 6 x 900 seconds
Hα 9 x 1200 seconds (-20°C) |
Camera: |
SBIG STL11000 with Astronomik type II-filters |
Optics/
Instrument: |
Astro-Physics 175mm f/8 StarFire EDF triplet refractor with flattener on AP1200 GTO |
|
Guiding: Lodestar attached to a 61mm-finder,
focusing: Robofocus and FocusMax,
image acquisition: CCD-Commander and MaximDL 5,
calibration and processing: PixInsight 1.8 |
Nevertheless the HαLRGB-version is interesting, it gives the nebula a different character.
Eta Carinae-complex (Carina), Hα-frame
Click on the image for a larger version
Date/Site: |
30. and 31. January 2014, Astrofarm at the Hacienda los Andes, Chile |
Exposure/
Filter |
Hα 9 x 1200 seconds (-20°C) |
Camera: |
SBIG STL11000 with Astronomik type II-filters |
Optics/
Instrument: |
Astro-Physics 175mm f/8 StarFire EDF triplet refractor with flattener on AP1200 GTO |
|
Guiding: Lodestar attached to a 61mm-finder,
focusing: Robofocus and FocusMax,
image acquisition: CCD-Commander and MaximDL 5,
calibration and processing: PixInsight 1.8 |
The pure Hα-channel in b/w.
|