Free Access

Table 5

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]

05 HE0036–5133 33.5 1300 6.6 38.1a
08 HE0045–2145 36.2 682 6.0
11 HE0103–5842 36.2 1729 6.8 37.7
16 HE0119–0118 34.4 3200 7.9 36.8 4192 7.9 38.0
31 HE0323–4204 34.2 3200 7.8 36.8 3030 7.6 38.0
80 HE2112–5926 33.5 2900 7.4
81 HE2128–0221 33.1 1800 6.7 36.5 1485 7.0 37.7
82 HE2129–3356 34.2 5000 8.2 36.5 5197 7.9 38.5
83 HE2204–3249 34.4 4000 8.1 36.9 5770 8.2 38.7
84 HE2211–3903 34.4 3900 8.0 38.0
85 HE2221–0221 35.2 4300 8.5

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).

(a)

HE0036 is an X-ray transient source (Grupe et al. 1995) and was at its peak luminosity during the ROSAT observations.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.