^ 1.01.11.2. Results for Palomar 5. [2006-11-17]. (原始内容存档于2016-03-15).
^Hessels, J. W. T.; et al, A 1.4 GHz Arecibo Survey for Pulsars in Globular Clusters, The Astrophysical Journal, November 2007, 670 (1): 363–378, Bibcode:2007ApJ...670..363H, S2CID 16914232, arXiv:0707.1602, doi:10.1086/521780.
^Boyles, J.; et al, Young Radio Pulsars in Galactic Globular Clusters, The Astrophysical Journal, November 2011, 742 (1): 51, Bibcode:2011ApJ...742...51B, S2CID 118649860, arXiv:1108.4402, doi:10.1088/0004-637X/742/1/51.
^Martell, S. L.; Smith, G. H.; Grillmair, C. J. A New Age Measurement for Palomar 5. American Astronomical Society, 201st AAS Meeting, #07.11; Bulletin of the American Astronomical Society. 2002, 34: 1103. Bibcode:2002AAS...201.0711M.
^Ibata, Rodrigo; Gibson, Brad. The Ghosts of Galaxies Past. Scientific American. April 2007, 296 (4): 40–45. Bibcode:2007SciAm.296d..40I. ISSN 0036-8733. PMID 17479629. doi:10.1038/scientificamerican0407-40.
^Chen, C. W.; Chen, W. P., Morphological Distortion of Galactic Globular Clusters, The Astrophysical Journal, October 2010, 721 (2): 1790–1819, Bibcode:2010ApJ...721.1790C, doi:10.1088/0004-637X/721/2/1790
N-body simulation of the Galactic globular cluster Palomar 5 and its stream, [2021-07-08], arXiv:2102.11348, doi:10.1038/s41550-021-01392-2, (原始内容存档于2021-12-18) (英语)