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Date: Tue, 23 Sep 2003 10:02:11 +0200 From: "Berto Monard" <lagmonar@csir.co.za> Subject: Re: re IGR J17544-2619 candidate Hi John and Taichi, My comments were meant off-list, Taichi.. ;-) >From what John wrote after all that processing, this actual B star might be the X emitter after all. Perhaps V838 Mon was similar at one stage... One could also consider the possiblility of a dust enriched HMXB (perhaps Be) near periastron.... but does the X spectrum and burst durations match the events? Is this an emission line source? Regards, Berto I might do some more follow up later (I probably forget), but spectral measures might be more indicative in this case
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