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.
Furuya R, Cesaroni R, Codella C, Testi L, Bachiller R, Tafalla M (2002). G24.78+0.08: A cluster of high-mass (proto)stars. ASTRONOMY & ASTROPHYSICS, 390, 1-4.
G24.78+0.08: A cluster of high-mass (proto)stars
Testi L;
2002
Abstract
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.File in questo prodotto:
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