Attendees: Fred, Sasha, Adam, Timea, HongLi, Mélanie, Fabrice, Nichol, Josh, Fabien, Nathalie, Leo, Yohan, Allison, Sylvain, Amy, Cara, Tapas, Mélisse
Minutes from our last telecon
Activities of the Core Working Group
Members and their main interests
NH3, 3’’ → T(NH3) of the cores surrounding (+ ALMA 0.2’’ @ 1mm)
Mean temperatures: 20K (SE or W51-E) 60K (W51-E) up to 120K (W51-IRS2)
Effect of the dynamic assumptions for temperature on the CMF: slightly steeper
Cores located on the extended free-free emission could correspond to chance alignment (no T measurements) or free-free peaks.
To remember: apply for more NH3 measurements at the VLA deadline for C configuration (later than August).
getsf seems to provide better flux estimates for the weakest sources. → better for mass studies
Gemma: W51-E (more sensitive and larger area than the paper to be submitted by Josh+)
Hongli G353.41 (CMF, fragmentation)
Nichol+Jeff?: on the denoised images by MnGSeg