The NGC/IC Project

NGC 4559

DSS Image annotation ©Copyright 1996 through 2008 by Robert E. Erdmann, Jr. - All rights reserved.
Commercial use of these images (books, software, etc.) is strictly prohibited without written permission.

Digitized Sky Survey (DSS) Image Information for  NGC 4559
DSS Acknowledgement ,  DSS Copyright Notice DSS Image Generation:  1st Generation DSS Image
Image Center (2000):  12h 35m 57.7s; +27º 57' 35"Image File Name:  n4559.jpg
Image Size (arcminutes):  10' x 10'Image Size (pixels):  353 x 353
Original NGC Catalogue Data for  NGC 4559
General Catalogue Designation:  3101William Herschel Designation:  I 92
John Herschel Designation:  1352Other Observers:  ...
Right Ascension (Equinox 1860):  12h 29m 00sAnnual RA Precession (Equinox 1880):  +2.98s
North Polar Declination (Equinox 1860):  61° 16.1'Annual DEC Precession (Equinox 1880):  +19.9"
Summary Description:  vB, vL, mE 150°, gbM, 3 st f
Notes:  Comments:  
Discovered by:  Friedrich Wilhelm Herschel (1738 - 1822)Year of Discovery:  1785
Telescope Aperture (Inches):  18.7Telescope Type:  Reflector
Understanding the 'Summary Description':  Summary Description Abbreviations List
Contemporary/Current Data for  NGC 4559
Right Ascension (2000):  12h 35m 57.7sDeclination (2000):  +27º 57' 35"
Object Type:  GalaxyObject Classification:  Sc II-III
Constellation:  Coma BerenicesPosition Angle:  150 °
Visual Magnitude:  9.8Surface Brightness:  13.9
Blue Magnitude:  10.3Object Size:  10.7'X4.4'
Also Cataloged As:  UGC 7766, MCG+05-30-030, H I-92, h 1352, GC 3101,
CGCG 159.024, IRAS 12334+2814, PGC 42002
Catalogue Notes:  ---------------
Book / Chart References for NGC 4559
Luginbuhl & Skiff (Page):  85Burnham's (Volume : Page):  ------
Uranometria 2000:  108,149,148Herald-Bobroff Astroatlas:  C-29,C-30
Microsky:  322GSC Small Region Number:  1992
POSS Blue Plate #:  64POSS Red Plate #:  64
Database Update Level: 2 (Complete)
Contemporary Visual Observation(s) for NGC 4559
NGC 4559 = UGC 07766 = MCG +05-30-030 = CGCG 159-024 = PGC 42002
12 35 57.7 +27 57 36
V = 10.0;  Size 10.7x4.4;  SB = 14.0;  PA = 150d

17.5": bright, large, elongated 5:3 NW-SE, ~7'x3'.  Exhibits a striking, unusual 
appearance with a broad, weak concentration to a large, elongated core.  The 
overall surface brightness is noticeably irregular with hints of brighter and 
darker spots.  The outer halo has a low surface brightness, particularly on the 
SE end which is cradled by three mag 12-12.5 stars.  This end is wider than the 
NW side, shows no tapering and there appears to be mottling near the 
superimposed stars.  IC 3550-52, IC 3555, and IC 3563 are HII regions and/or 
star clouds within N4559 discovered by Wolf (made no attempt to identify).

- by Steve Gottlieb

Historical Research Notes / Correction for NGC 4559
NGC 4559.  IC 3550, 51, 52, 55, and 63 are HII regions in the arms of this
galaxy, found on a Heidelberg plate by Max Wolf.  IC 3554 and 3564 are stars
superposed on the galaxy.  See the IC numbers for a bit more information.
 - Dr. Harold G. Corwin, Jr.
Correction Disclaimer
As with all corrections to the NGC and IC Catalogues, there is a certain margin
for error, even though the evidence supporting the correction may be strong and
compelling. It is with this in mind that we ask the user to use this information
as 'Most Probable', but never to assume the correction is 'Absolute'.  All
published corrections are based on an exhaustive 'paper chase' of the historical
record back to the original discoverer's published notes/papers, and are
therefore based upon the historical accuracy (or inaccuracy) of those particular
notes/papers. In short, Caveat Emptor! - Robert E. Erdmann, Jr.
Data Sources Used to research NGC 4559
[NGC] New General Catalogue / [IC] Index Catalogue (Dreyer - 1888, 1895, 1908)
[OHCDSO] Observing Handbook and Catalog of Deep-Sky Objects (Luginbuhl & Skiff - 1990)
[RE-NGCDDB] NGC Discoverer's Database (Erdmann 1990 - 2006)
[UGC] Uppsala General Catalog of Galaxies (Nilson - 1973)
[CGCG] Catalog of Galaxies & Clusters of Galaxies (Zwicky - 1968)
[MCG] Morphological Catalog of Galaxies (Vorontsov-Velyaminov et al - 1962 thru 1968)
[RE-AZDB] The Arizona Database®, V15.5 (Erdmann - 1987 thru 2006)
[HC-PPL] NGC/IC Accurate Positions List Database (Corwin - 1996 thru 2006)
[SG-NGCO] NGC/IC Observations Database (Gottlieb - 1998 thru 2006)
[PGC] Principle Galaxy Catalog (Paturel et al. - 1989, 2003)
[DSS] Digitized Sky Survey - 1st (102 CD-ROM) and 2nd (Web Site) Generation (STScI - 1994)
[NED] NASA's Extragalactic Database (NED) located at http://nedwww.ipac.caltech.edu/

Additional Notes
1st generation images were generated from the 102 CD-ROM version of the Digitized Sky Survey (DSS)
2nd generation images were generated at the DSS web site located at http://archive.stsci.edu/cgi-bin/dsswin
Luginbuhl & Skiff page numbers are from 'Observing Handbook and Catalogue of Deep-Sky Objects' by Christian B. Luginbuhl and Brian A. Skiff, produced by Cambridge University Press
Burnham's refers to 'Burnham's Celestial Handbook' in three volumes produced by Dover Publications, Inc.
Uranometria 2000 chart numbers are for those printings authored by Tirion, Rappaport & Lovi, and are not for the most recent printings authored by Tirion, Rappaport & Remaklus in which the charts were re-numbered, all of which were and/or are produced by Willmann-Bell, Inc.
The Herald-Bobroff Astroatlas is by D. Herald and P. Bobroff of Canberra, Australia and is produced by HB2000 Publications
Microsky® is the microfiche rendition of the Palomar Observatory Sky Survey (POSS) produced by Deen Publications (P.O. Box 867088; Plano Texas 75086)
POSS refers to the Palomar Observatory Sky Survey produced by The National Geographic Society in conjunction with The California Institute of Technology
All DSS image annotation was performed by Robert E. Erdmann, Jr., and is ©Copyright 1996 through 2008 by Robert E. Erdmann, Jr. - All rights reserved
All product names, trademarks, and copyrights are the property of their respective owners
Contemporary/Current Data for this object was hand collected and entered from the data sources listed in the "Data Sources Used" section of this table above.- Robert E. Erdmann, Jr.


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