12:05:36	 From Annie Zavagno : What kind of pressure do you observed in the stripped gas and do you see star formation in the stripped parts ?
12:06:27	 From Claude Carignan : This was the idea of the Subaru data. We found no SF in the clouds.
12:07:19	 From Claude Carignan : ...which eliminates a possible merger.
12:07:50	 From Annie Zavagno : Do you think that observing no SF is due to an evolution effect (not enough density yet?)
12:08:15	 From Francois Hammer : And the pressure is sufficient to move the whole gas of WLM when compared to stars.
12:13:10	 From Guillaume BONNET  To  Annie Zavagno(privately) : Annie, does he answer to your questions ?
12:17:09	 From Annie Zavagno  To  Guillaume BONNET(privately) : non, pas sur l'aspect évolutif mais ce n'est pas grave, ni sur la valeur de la pression, mais là aussi, pas grave. Merci d'avoir demandé. Annie