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

被引：31
作者：
Furuya, RS
Cesaroni, R
Codella, C
Testi, L
Bachiller, R
Tafalla, M
机构：
[1] INAF, Osservatorio Astrofis Arcetri, I-50125 Florence, Italy
[2] CNR, Ist Radioastron, Sez Firenze, I-50125 Florence, Italy
[3] Observ Astron Nacl IGN, Madrid 28800, Spain
来源：
ASTRONOMY & ASTROPHYSICS | 2002年 / 390卷 / 01期
关键词：
stars : formation; radio lines : ISM; ISM : jets and outflows; ISM : individual objects : G24.78+0.08;
D O I：
10.1051/0004-6361:20020850
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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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收藏
页码：L1 / L4
页数：4
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