G24.78+0.08: a cluster of high-mass (proto)stars
R.S. Furuya, R. Cesaroni, C. Codella, L. Testi, R. Bachiller, M. Tafalla
We present the results of high angular resolution
observations at millimeter wavelengths of the high-mass star
forming region G24.78+0.08, where a cluster of
four young stellar objects is detected.
We discuss evidence for these to be high-mass
(proto)stars in different evolutionary phases.
One of the sources is detected only in the continuum at 2 and 2.6~mm and
we suggest it may represent a good candidate of a high-mass protostar.