A Method for Obtaining the Nuclear Component in Active Galaxies

Details A Method for Obtaining the Nuclear Component in Active Galaxies A Method for Obtaining the Nuclear Component in Active Galaxies

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..119s&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 119-122 (1998).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We present a new method for the obtention of the nuclear component of active galatic nuclei, that relies on the convolution of a two-dimensional model of the host galaxy, based on seeing-free morphological parameters, with the seeing PSF. The procedure overcomes some limitations of the methods currently in use and does not assume that the nucleus is unresolved.

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