Additional Newly Identified Star Clusters in M31

作者:Krienke O Karl*; Hodge Paul W
来源:Publications of the Astronomical Society of the Pacific, 2013, 125(928): 636-638.
DOI:10.1086/671227

摘要

Using the HSTarchives, we have searched portions of the southern half and northwest quarter of the Andromeda Galaxy (M 31, NGC 224) for previously unrecognized star clusters. The result is a table of the characteristics of 71 newly identified star clusters. Most are moderately faint, low-mass clusters. Absolute magnitudes range from M(V)=-6.3 to-2.5.

  • 出版日期2013-6