Abstract
A classification method has been developed for early—type stars observed on the Dominion Astrophysical Observatory photometric system. Two reddening—independent parameters, Q(35) and Q(38), are used. Q(35) is a measure of the Balmer discontinuity, while Q(38) is a measure of the strength of the upper members of the Balmer series. A preliminary calibration of Q(35) and Q(38) in terms of spectral types and luminosity classes is given, and applications to several groups of stars are shown.
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Morris, S.C., Hill, G., Walker, G.A.H., Thompson, H.I.B. (1973). Classification of Early Type Stars on the Dominion Astrophysical Observatory Photometric System. In: Fehrenbach, C., Westerlund, B.E. (eds) Spectral Classification and Multicolour Photometry. International Astronomical Union / Union Astronomique Internationale, vol 50. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2627-7_29
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DOI: https://doi.org/10.1007/978-94-010-2627-7_29
Publisher Name: Springer, Dordrecht
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