Publication Date:
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.
Iris type:
01.01 Articolo in rivista
Keywords:
Astronomia Galattica; Radioastronomia
List of contributors: