G24.78+0.08: A cluster of high-mass (proto)stars
Published Jul 1, 2002 · R. S. Furuya, R. Cesaroni, C. Codella
Astronomy and Astrophysics
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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 dierent 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.
Study Snapshot
Key takeawayA cluster of four young stellar objects in the high-mass star forming region G24.78+0.08 is likely composed of high-mass (proto)stars in different evolutionary phases.
PopulationOlder adults (50-71 years)
Sample size24
MethodsObservational
OutcomesBody Mass Index projections
ResultsSocial networks mitigate obesity in older groups.