The Young Stellar Population in M17 Revealed by Chandra

The Young Stellar Population in M17 Revealed by Chandra
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DOI：
10.1086/512068
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发表时间：
2006-12
期刊：
The Astrophysical Journal Supplement Series
影响因子：
--
通讯作者：
P. Broos;E. Feigelson;L. Townsley;K. Getman;Junfeng Wang;G. Garmire;Zhibo Jiang;Y. Tsuboi
P. Broos;E. Feigelson;L. Townsley;K. Getman;Junfeng Wang;G. Garmire;Zhibo Jiang;Y. Tsuboi
中科院分区：
其他
文献类型：
--
作者：
P. Broos;E. Feigelson;L. Townsley;K. Getman;Junfeng Wang;G. Garmire;Zhibo Jiang;Y. Tsuboi

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我们在这里报告了Chandra ACIS对M17H II区域及其周围恒星群的观测结果。该场揭示了观测到的X射线亮度(未经吸收校正)在~29.3ergs S-1&lt；32.8ergs S-1之间的886个源，其中771个在红外图像中有恒星对应。除了X射线源性质的综合表格外，还提供了几个结果：
We report here results from a Chandra ACIS observation of the stellar populations in and around the M17 H II region. The field reveals 886 sources with observed X-ray luminosities (uncorrected for absorption) between ~ 29.3 ergs s-1 < log LX < 32.8 ergs s-1, 771 of which have stellar counterparts in infrared images. In addition to comprehensive tables of X-ray source properties, several results are presented: