Evidence for Relativistic Outflows in Narrow-line Seyfert 1 Galaxies

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Scientific paper

We report the observation of features near 1 keV in the ASCA spectra from three ``Narrow Line Seyfert 1'' (NLS1) galaxies. We interpret these as oxygen absorption in a highly relativistic outflow. If interpreted as absorption edges, the implied velocities are 0.2--0.3 c, near the limit predicted by ``line-locking'' radiative acceleration. If instead interpreted as broad absorption lines, the implied velocities are ~ 0.57 c, interestingly near the velocity of particles in the last stable orbit around a Kerr black hole, although a physical interpretation of this is not obvious. Interpretation in the context of a relativistic wind is supported by the fact that narrow-line Seyfert 1 galaxies share many optical emission-line and broad band properties with broad absorption line quasars. Many of these objects show strong or extreme Fe II and weak [O III] emission, have red continuum spectra and relatively strong infrared emission, and both classes are predominately radio quiet.

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

Evidence for Relativistic Outflows in Narrow-line Seyfert 1 Galaxies 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 Evidence for Relativistic Outflows in Narrow-line Seyfert 1 Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evidence for Relativistic Outflows in Narrow-line Seyfert 1 Galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1177295

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