Music Hall of Williamsburg. Comparison of the virial products measured from SE spectra and rms spectra. I don't know what to do to help!!?? Ideally, the luminosity variability should be four times as large as the line-width variability 0. It may even be cute when they lick your ice cream cone. The three components were varied simultaneously with six free parameters:
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Each line profile is normalized by the maximum value of the fit. You must log in or sign up to reply here. However, due to the observational challenges of reverberation mapping campaigns, fewer than 50 BH masses have been measured to date using this technique Wandel et al. By-the-way…my comment to you about eating your butthole was just a joke and I never eat gravy! Im sorry but that just made me sick. For example, Shields et al.
For consistency with other studies on the reverberation and SE masses, we focus on the line-width measurements from the fits in the rest of the paper unless explicitly noted. Daeseong Park et al ApJ SerenityRick , Aug 8, In a sense, these new estimators can be thought of as introducing a line-width dependent virial factor to correct for the systematic difference of the geometry and kinematics of the gas contributing to the SE line profile and that contributing to the rms spectra. These results are similar to the findings by Collin et al. John Smoltz Qualifies for Senior U.