HD 93607 is a B4main sequence star, although older spectral studies classified it as asubgiant.[7] It is included on a list of the least variable stars amongst those observed by theHipparcos satellite, with a possible variation less than 0.01magnitudes.[8]
HD 93607 lies in the core region of the brightopen cluster IC 3602. Its age is uncertain but around 17 million years.[5]
^abcMermilliod, J.-C (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)".Catalogue of Eggen's UBV Data.Bibcode:1986EgUBV........0M.
^Houk, N; Cowley, A. P (1975).University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90° to -53.0°.Bibcode:1975mcts.book.....H.
^abDavid, Trevor J; Hillenbrand, Lynne A (2015). "The Ages of Early-type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets".The Astrophysical Journal.804 (2): 146.arXiv:1501.03154.Bibcode:2015ApJ...804..146D.doi:10.1088/0004-637X/804/2/146.S2CID33401607.
^Skiff, B. A (2014). "VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications (Skiff, 2009-2016)".VizieR On-line Data Catalog: B/Mk. Originally Published in: Lowell Observatory (October 2014).1.Bibcode:2014yCat....1.2023S.
