A simple population synthesis model for the continuum of the Seyfert type-2 galaxy MK 348

Details A simple population synthesis model for the continuum of the Seyfert type-2 galaxy MK 348 A simple population synthesis model for the continuum of the Seyfert type-2 galaxy MK 348

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.157..125g&link_type=abstract

(Instituto de Astrofisica de Canarias and Comision Interministerial de Ciencia y Tecnologia, Summer School on Evolutionary Pheno

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Seyfert Galaxies, Spectral Energy Distribution, Star Formation, Stellar Spectra, Synthesis

Scientific paper

The spectral energy distribution of the Seyfert type-2 galaxy Mk 348 is analyzed based on IUE observations and published data. It is found that most of the optical and near-IR flux comes from the underlying galaxy bulge population. The rest of the emission can be fitted by a power law. In order to explain the X-ray emission, the power law requires either a change of slope or a cutoff before 2 keV. The possibility that the emission originates in a young star cluster is discussed, and a simple population synthesis model for the continuum of the galaxy is presented.

Affiliated with

Also associated with

No associations

Rating

A simple population synthesis model for the continuum of the Seyfert type-2 galaxy MK 348 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A simple population synthesis model for the continuum of the Seyfert type-2 galaxy MK 348, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A simple population synthesis model for the continuum of the Seyfert type-2 galaxy MK 348 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1703517