*** Abell 2199 ***
|Figure 1 - Central region of A2199. The brightest galaxy in this image is NGC6166. Image from the STScI Digitized Sky Survey. Width is 15' and North is up.|
Download the finder chart I've created for the central 1º X 1º field.
Uranometria 2000.0 shows a close up plot of A2199 on chart A3. A dashed circle with a radius less than 1º indicates the location and size. As with other galaxy clusters, I tried to answer three questions.
The observing list is contained in Table I – Galaxies within 1º of the center of Abell 2199.
The headings of the columns in Table I are described in Table II below.
Table II - Description of headings in Table I
|Name||Generally the most common catalog name.|
|Alternate name 1||
Identification in an alternate catalog.
|Alternate name 2||Identification in an alternate catalog.|
|RA||Right Ascension for Equinox 2000 in hours, minutes, and seconds.|
|DEC||Declination for Equinox 2000 in degrees, arc minutes, and seconds.|
|Magnitude||For most of the data, this is the photographic apparent magnitude.|
|R (arcmin)||Distance of galaxy from center of cluster in arcmin.|
|Radial velocity||Reported heliocentric radial velocity in km/sec.|
|Cluster member?||Remarks indicating likelihood of being a cluster member.|
|Date observed||Date of most recent observation with my 17.5" f/4.5 reflector.|
|Magnification||The magnification used for the reported observation|
|% averted vision||The percentage of time I could hold the object with averted vision.|
You’ll notice several designations in Table I, including objects from NGC, IC, UGC, MCG, CGCG, and PGC catalogs. However, some less common designations are also used. Full names for these other designations are shown in Table III.
Table III - Some less common object designations.
|KUG||Kiso Ultraviolet Galaxy Catalogue|
|MAPS-NGP||Minnesota Automated Plate Scanner - North Galactic Pole|
|AGC||Arecibo General Catalog|
|2MASX||2 Micron All Sky Survey Extended Objects|
|ABELL||Abell Clusters of Galaxies|
|ARK||Arakelian Emission Line Objects|
Preparation is very important. The most useful charts are those I prepared from STScI Digitized Sky Survey images of the central 1º X 1º field and selected outlying areas. I labeled the target galaxies in Photoshop. For use in the field, I print out charts of regions approximately 20' X 30'. Feel free to download the finder chart I've created for the central 1º X 1º field.
Although a large number of galaxies are clustered together in the central 1º, using a low power, wide field eyepiece will show very few at one time. Most of them are very small and faint. Higher magnification improves contrast and shows more detail. For observing faint, low contrast galaxies, I find using an exit pupil of approximately 1 - 1.5mm provides the optimum view. For my 17.5" scope, I generally use a 7.5mm Takahashi LE or 7mm Nagler T6 eyepiece, providing magnifications of 267X and 286X, respectively. For viewing the smallest and faintest galaxies, and for splitting the very close galaxy pairs, the 5mm Takahashi LE, providing 400X, works best. Detecting the faintest members also requires very dark skies with good to excellent transparency.
Most of the galaxies on the observing list are faint. Most of the recorded descriptions are brief. In order to provide some indication of the relative difficulty of seeing an object, I record the magnification used for the observation and the percentage of time I was able to hold the object with averted vision. Any object that I could hold less than 50% of the time is very challenging.
Selected Observing Notes
Currently I've observed 99 objects on the list. At least six are likely not members of the cluster. Seven also appear on the Abell 2197 list.
Creating a database for "The Sky"
If you have questions, or want to report any errors, please contact me at: ahighe @ ix.netcom.com.
I also would appreciate hearing about your observations, especially if you use a scope of a different size. Thanks.
Return to Home Page
Copyright © 2003 by Albert Highe, unless otherwise noted. All rights reserved.
This page accessed times.
Page created by: ahighe @ ix.netcom.com
Changes last made on: November 26, 2003