Table 1
X-ray observation for SNe Iax.
| t | Distance | LX | Ṁ | ||
| Name | [days] | [Mpc] | [1038 erg / s] | [10-5M⊙/yr] | |
| (1) | (2) | (3) | (4) | ||
|
|
|||||
| 2005hk | 187.0 | 56 | <39.3 | <13.1 | <9.3 |
| 2008A | 53.5 | 70 | <89.5 | <10.7 | <7.5 |
| 2008ae | 9.26 | 127 | <434 | <9.8 | <6.9 |
| 2008ge | 23.2 | 16 | <19.3 | <3.3 | <2.3 |
| 2008ha | 36.4 | 22.5 | <26.8 | <4.8 | <3.4 |
| 2010ae | 17.4 | 17 | <22.5 | <3.1 | <2.2 |
| 2010el | 9.5 | 30.19 | <585.4 | <11.5 | <8.1 |
Notes. SNe Iax were observed by the Swift X-Ray Telescope (XRT). The data used here obtained from Russell & Immler (2012). (1) t is the time after outburst (see Russell & Immler 2012); (2) 3σ upper limit to the 0.2–10 KeV X-ray band luminosity; (3) upper-limit mass-loss rate of the progenitor system (for wind velocity of υwind = 100 km s-1), for which a power law index of the SN ejecta of n = 10 and υs = 10 000 km s-1 are adopted; (4) similar to (3), but for υs = 5000 km s-1 case.
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