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Paper: Characterizing Classical Be Stars via Intermediate-band Photometry
Volume: 508, The B[e] Phenomenom: Forty Years of Studies
Page: 51
Authors: Kaltcheva, N.; Golev, V.
Abstract: Photometry-based determination of physical parameters of classical Be stars is useful to clarify their evolutionary status and their presence in star-forming complexes and open clusters. We use a sample of nearly 600 stars with complete uvbyβ data to evaluate various methods for providing estimates of absolute magnitude and color excess for O- and B-type emission-line objects.
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