BH mass estimates from the broad Paα line compared with A. Schulze’s BH mass estimates from Hα.
|Source||log (LPaα [ W ])||FWHM Paα||log (MBH/M⊙)||log (L5100 [ W ])||FWHM Hα||log (MBH/M⊙)||log (Lbol [ W ])|
|[km s-1]||[km s-1]|
Notes. Bolometric luminosities are derived from ROSAT soft X-ray luminosities. The bolometric luminosities are derived from the unabsorbed ROSAT fluxes (Mahony et al. 2010), using a bolometric correction factor of ~50 (Hopkins et al. 2007).
HE0036 is an X-ray transient source (Grupe et al. 1995) and was at its peak luminosity during the ROSAT observations.
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