Figure 2.
Comparison of observed periods in rest-frame versus the characteristic periods of accretion discs. Panels (a, b, c, d) are the Keplerian periods at the region for 5100 Å photons (T5100), the critical radius of self-gravity (TSG), averaged radius (Tmean) and the precessing period of warped discs (TWD) versus observed periods(Tobs), respectively. Their corresponding histograms are shown in panels (e, f, g, h). Vertical dash lines are the average levels.

Comparison of observed periods in rest-frame versus the characteristic periods of accretion discs. Panels (a, b, c, d) are the Keplerian periods at the region for 5100 Å photons (T5100), the critical radius of self-gravity (TSG), averaged radius (Tmean) and the precessing period of warped discs (TWD) versus observed periods(Tobs), respectively. Their corresponding histograms are shown in panels (e, f, g, h). Vertical dash lines are the average levels.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close