SDSS J2125-0813: the evidence for the origination of optical FeII emission lines from an accretion disc near a central black hole

Details SDSS J2125-0813: the evidence for the origination of optical FeII emission lines from an accretion disc near a central black hole SDSS J2125-0813: the evidence for the origination of optical FeII emission lines from an accretion disc near a central black hole

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006mnras.372l...5z&link_type=abstract

Monthly Notices of the Royal Astronomical Society: Letters, Volume 372, Issue 1, pp. L5-L8.

Astronomy and Astrophysics

Astronomy

6

Galaxies: Active: Quasars: Emission Lines: Accretion, Accretion Discs, Galaxies: Active, Quasars: Emission Lines, Accretion

Scientific paper

We report on the radio-quiet quasar SDSS J2125-0813 which obviously emits optical FeII emission lines and double-peaked broad Balmer emission lines. Using the accretion disc model for double-peaked, broad, low-ionization emission lines, we reproduce the composite line spectra at the optical band between 4100 and 5600 Å. Broad FeII emission lines can be fitted simultaneously with the broad Hβ and MgI lines, such that all broad lines have an elliptical disc profile with the same disc parameters. This result indicates that the optical FeII emission lines originate from the accretion disc near the central black hole which produces the double-peaked broad Balmer emission lines. Furthermore, we find that the object has a dimensionless accretion rate , which is much larger than the accretion rate for the advection-dominated accretion flow (ADAF) mode, and that the energy budget of the accretion disc is enough to power the double-peaked broad Balmer emission lines.

Affiliated with

Also associated with

No associations

Rating

SDSS J2125-0813: the evidence for the origination of optical FeII emission lines from an accretion disc near a central black hole 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 SDSS J2125-0813: the evidence for the origination of optical FeII emission lines from an accretion disc near a central black hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SDSS J2125-0813: the evidence for the origination of optical FeII emission lines from an accretion disc near a central black hole will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1427670