G24.78+0.08: A cluster of high-mass (proto)stars

R. S. Furuya, R. Cesaroni, C. Codella, L. Testi, R. Bachiller, M. Tafalla
2002 Astronomy and Astrophysics  
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.
doi:10.1051/0004-6361:20020850 fatcat:qxelhudewnfgxj3lhnmrfs3t3u