The Active Nucleus in NGC 4579

Details The Active Nucleus in NGC 4579 The Active Nucleus in NGC 4579

2010-06-25

arxiv.org/abs/1006.4896v1

2010IAUS..267..123M

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

1 page, 1 figure

Scientific paper

10.1017/S1743921310005843

In this work, we present an analysis of a data cube obtained with the instrument IFU/GMOS Gemini North telescope centered 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.

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