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).
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.