Table 1
XMM-Newton/RGS observations used in this paper.
| Source | IDa | t (ks)b | z | O vi | O viitot | O viisim |
|
|
||||||
| IC 1459 | 0135980201 | 26 | 0.006 | Y | 2.5 | 1.5 |
|
|
||||||
| M 84 | 0673310101 | 64 | 0.0034 | Y | 3.7 | 3.4 |
|
|
||||||
| M 86 | 0108260201 | 91 | –0.0009 | P | 4.1 | 6.5 |
|
|
||||||
| M 89 | 0141570101 | 29 | 0.001 | P | 3.1 | 3.3 |
|
|
||||||
| NGC 1316 | 0302780101 | 166 | 0.0059 | Y | 6.3 | 6.7 |
| 0502070201 | ||||||
|
|
||||||
| NGC 1332 | 0135980201 | 64 | 0.0052 | UL | 2.1 | 1.6 |
|
|
||||||
| NGC 1404 | 0304940101 | 29 | 0.0065 | UL | 2.0 | 2.0 |
|
|
||||||
| NGC 4636 | 0111190101 | 102 | 0.0037 | Y | 5.0 | 6.0 |
| 201/501/701 | ||||||
|
|
||||||
| NGC 5846 | 0021540101/501 | 195 | 0.0061 | Y | 3.6 | 3.7 |
| 0723800101/201 | ||||||
Notes. O vi detections are taken from Bregman et al. (2005): Y = yes, P = possible, UL = upper limits. O vii combined significance in units of σ: 21.6 Å and 22.1 Å significance added in quadrature (tot) and simultaneous fit (sim) with f21.6 / 22.1 ≡ 1.3 as predicted by our thermal model (see Table 2 and Sect. 3.1).
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