Messier 58 (also M58, NGC 4579, IRAS 12351+1205, MCG 2-32-160, UGC 7796 and PGC 42168) is a magnitude +10.5 barred spiral galaxy located 62 million light-years away in the constellation Virgo.
The galaxy was discovered by French astronomer Charles Messier on the 15th April 1779.
Right Ascension 12h 37m 43.5s, Declination +11° 49' 05"
Title: The Active Nucleus in NGC 4579 Authors: Roberto B. Menezes, Joćo E. Steiner, Tiago V. Ricci, Alexandre S. Oliveira
In this work, we present an analysis of a data cube obtained with the instrument IFU/GMOS Gemini North telescope centred on the nuclear region of the LINER galaxy NGC 4579. This galaxy is known to have a type 1 AGN (see Eracleous et al. 2002 for a review). The methodology used for the analysis of the data cube was PCA tomography (Steiner et al. 2009), which consists of applying the statistical tool known as principal component analysis (PCA) to extract information from data cubes.