NGC 4559 in Coma Berenices
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ON IMAGE FOR FULL SIZE VIEW
(2800x2100)
Scope:
Celestron 9.25 Edge 235 mm at f/7, Location: DAA Observatory, Shelter Valley CA,
30 March 2019
Camera: ST8300M (Baader LRGB filters) Exposure:
Exposure: 16 x 12 min (2x2 bin) exposure with IR/UV Block filter, 10 x 5 min
(2x2 bin) RGB exposures. Processing: Data
Collection - Sequence Generator Pro (as FITs). Exposure calibration,
LRGB registration, and stacking (Median combine - Winsorized Sigma
Clipping) - PixInsight. LRGB channel registration,
equalization and gradient removal - PixInsight. Curves, Levels, RGB
combine, Luminance layering - PixInsight. Final finishing -
Photoshop. Annotation - Photoshop and PixInsight. RGB calibration - eXcalibrator. This image is a RGB combine
with Luminance layering. Images processed at 3352 x 2532 resolution. Final Image size is approximately
2800 x 2100. North is up in this image. The
dominant galaxy in this image is NGC 4559. It is classified SAB(rs)cd -
barred galaxy with spiral and ring features. It is about 24 to 36 million light
years distant. NGC 4559 is a member of the Coma I group and several larger
groups [CHM2007] LDC 709 and LDC 867. Also in this image are galaxies IC
3598 and IC 3592. The latter (IC 3592) is also known as NGC 4559A - but it is
much more distant (at 334 million light years) than the main NGC 4559 galaxy and
is not interacting. There are numerous other background galaxies in this
image - some of which are indicated in the annotated
image. These galaxies range in distance from 333 to 1,447 million light
years distant. These galaxies and some of the brighter
stars are identified in the annotated
image.. This image replaces an earlier image located in the Archives
here. Horizontal FOV is
approximately 38 arc minutes (0.81 arcsec/pix image scale on the full size
image). Image center is located approximately - Equatorial 2000: RA: 12h 36m 13s Dec: +28°01'48"
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