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Paper: G24.78+0.08: A Cluster of High Mass (Proto)Stars
Volume: 287, Galactic Star Formation Across the Stellar Mass Spectrum
Page: 237
Authors: Furuya, R. S.; Cesaroni, R.; Testi, L.; Codella, C.
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.
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