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

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

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...390l...1f&link_type=abstract

Astronomy and Astrophysics, v.390, p.L1-L4 (2002)

Astronomy and Astrophysics

Astrophysics

23

Stars: Formation, Radio Lines: Ism, Ism: Jets And Outflows, Ism: Individual Objects: G24.78+0.08

Scientific paper

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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