... eruption[*]
Appendix A is only available in electronic form at http://www.edpsciences.org
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... spectrum[*]
The difference in the blackbody temperature between Lynch et al. (2004) and the present study (2700 K versus $\sim $5000 K) is simply due to the interstellar reddenning correction, i.e. no reddenning correction in Lynch et al, versus EB-V = 0.9 in the present study. Indeed, if we apply our fitting procedure with EB-V = 0.0 to the ${\it JHKLM}$ magnitudes of Lynch et al. in January 2002, the resultant temperature is $\sim $2700 K.
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Copyright ESO 2005