Volume 390, Number 1, July IV 2002
|Page(s)||L1 - L4|
|Published online||05 July 2002|
Letter to the Editor
G24.78+0.08: A cluster of high-mass (proto)stars
Osservatorio Astrofisico di Arcetri, INAF, Largo E. Fermi 5, 50125 Firenze, Italy
2 Istituto di Radioastronomia, CNR, Sezione di Firenze, Largo E. Fermi 5, 50125 Firenze, Italy
3 Observatorio Astronómico Nacional (IGN), Apartado 1143, 28800 Alcalá de Henares (Madrid), Spain
Corresponding author: R. Cesaroni, email@example.com
Accepted: 6 June 2002
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.
Key words: stars: formation / radio lines: ISM / ISM: jets and outflows / ISM: individual objects: G24.78+0.08
© ESO, 2002
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