Chamaeleon

1994, Revista Mexicana de Astronomía y Astrofísica, Volumes 28-30, Instituto de Astronomía, Universidad Nacional Autónoma de México, page 50, The X-ray luminosity function has been determined so far only for the far only for the central parts of the Chamaeleon SFR by Fiegelson et al. (1993).

2001, A. Mizuno, T. Hayakawa, T. Onishi, Y. Fukui, Dense Core Survey toward the Chamaeleon Dark Cloud Complex with the NANTEN Radio Telescope, Alwyn Wootten (editor), Science with the Atacama Large Millimeter Array (ALMA): Proceedings of a Conference, Astronomical Society of the Pacific, page 146.

2005, Memorie Della Società Astronomica Italiana, Volume 76, Issues 1-2, Società Astronomica Italiana, page 263, We note, however, that the surveyed area in Chamaeleon II was relatively small in comparison with the other two regions, covering only part of a cloud core to the north-west.