Negative X-ray reverberation time delays from MCG-6-30-15 and Mrk 766

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Accepted for publication in MNRAS Letters. The paper (6 pages) contains 2 figures and 1 table

Scientific paper

We present an X-ray time lag analysis, as a function of Fourier frequency, for MCG-6-30-15 and Mrk 766 using long term XMM-Newton light curves in the 0.5-1.5 keV and the 2-4 keV energy bands, together with some physical modelling of the corresponding time lag spectra. Both the time lag spectra of MCG-6-30-15 and Mrk 766 show negative values (i.e. soft band variations lag behind the corresponding hard band variations) at high frequencies, around 0.001 Hz, similar to those previously observed from 1H 0707-495. The remarkable morphological resemblance between the time lag spectra of MCG-6-30-15 and Mrk 766 indicate that the physical processes responsible for the observed soft time delays is very similar in the two sources, favouring a reflection scenario from material situated very nearby to the central black hole.

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

Negative X-ray reverberation time delays from MCG-6-30-15 and Mrk 766 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 Negative X-ray reverberation time delays from MCG-6-30-15 and Mrk 766, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Negative X-ray reverberation time delays from MCG-6-30-15 and Mrk 766 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-34234

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