An accretion disk origin for the ultraviolet continuum in Seyfert 1 galaxies and quasars

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Accretion Disks, Continuous Spectra, Quasars, Seyfert Galaxies, Ultraviolet Astronomy, Ultraviolet Spectra, Astronomical Models, Galactic Nuclei

Scientific paper

For the last two decades, intensive studies have been conducted regarding the continuous emission from quasars and the nuclei of Seyfert 1 galaxies. Observations over at least three frequency octaves are needed for a meaningful analysis of the continuum. Recent satellite observatories have made it possible to obtain the required data. However, some observational problems had to be overcome in connection with the interpretation of the data. One of these problems is related to the observation that the starlight in many Seyfert galaxies is often at least as bright as the nonstellar continuum emitted in their nuclei. In the case of a few Seyfert 1 galaxies, such as Markarian 231, a study of the intrinsic continuum is virtually impossible, because the galaxies are heavily reddened. Questions regarding the accretion disk hypothesis are discussed, and observations which are crucial to an understanding of the accretion process are considered.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

An accretion disk origin for the ultraviolet continuum in Seyfert 1 galaxies and quasars 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 An accretion disk origin for the ultraviolet continuum in Seyfert 1 galaxies and quasars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An accretion disk origin for the ultraviolet continuum in Seyfert 1 galaxies and quasars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1508215

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.