DSS image of NGC2090
Digitized Sky Survey image of NGC2090, 30' x 30' with north at top and west to the right

DSS image of NGC2090
Overlaid DSS image of NGC2090, 30' x 30' with north at top and west to the right
2MASX J05470188-3415021, ESO 363- G 023, IRAS 05452-3416, PGC 017819

Type  Galaxy
Magnitude  11.2
Size  5' x 2.5' @ 13°
RA (2000)  5h 47' 1.9"
Dec (2000)  34° 15' 2" S
Constellation  Columba
Description  B, pL, iR, bgM, stellar N, cE 10 deg

Observing Notes

Andrew Cooper
30 Jan 2011 Hale Pohaku, HI (map)
46cm f/4.5 Newtonian, Deep Violet @ 175x

Small. bright, elongated 2:1 north-south, stellar core, no other structure noted

Andrew Cooper
17 Nov 2009 Hale Pohaku, HI (map)
46cm f/4.5 Newtonian, Deep Violet @ 262x

Small, elongated 3:1 north-south, modest brightening at center
Other Data Sources for NGC2090
Nearby objects for NGC2090
2 objects found within 120'
NGC2061 NGC2090
Acknowledgements and Credits...

Drawings, descriptions and CCD photos are copyright Andrew Cooper unless otherwise noted, no usage without permission. Use for non-profit and educational reasons is generally given on request.

Positional and some physical information is from the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.

Additional object data from the SIMBAD database, operated at CDS, Strasbourg, France.

The Digitized Sky Survey was produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope.

Dark nebulae data from E.E. Barnard, A Photographic Atlas of Selected Regions of the Milky Way. Ed. Edwin B. Frost and Mary R. Calvert. Carnegie Institution of Washington, 1927

Object descriptions of Rev. Webb from Celestial Objects for Common Telescopes sixth edition, Rev. T.W. Webb, 1917, edited by Rev T.E.Espin.