Multi-Epoch BVRI Photometry for Warm Hypergiants in M31 and M33

Evolved supergiants with A to G spectral types that show evidence for high mass loss and/or are very dusty. Some have [Fe II] or [O I] emission in their spectra.

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LGGSNameClassLast Measured V_magTableGraphVariability
Color composite thumbnail image of M31-004322.50J004322.50+413940.9M31-004322.50Warm-Hypergiant 19.07TableGraphVariability
Color composite thumbnail image of M31-004444.52J004444.52+412804.0M31-004444.52Warm-Hypergiant 18.13TableGraphVariability
Color composite thumbnail image of M31-004522.58J004522.58+415034.8M31-004522.58Warm-Hypergiant 18.60TableGraphVariability
Color composite thumbnail image of M31-004621.08J004621.08+421308.2M31-004621.08Warm-Hypergiant 17.97TableGraphVariability
Color composite thumbnail image of Var AJ013232.86+303025.2 Var AWarm-Hypergiant 18.46TableGraphVariability
Color composite thumbnail image of V-093351J013352.42+303909.6V-093351Warm-Hypergiant 16.60TableGraphVariability
Color composite thumbnail image of B324J013355.96+304530.6B324Warm-Hypergiant 14.81TableGraphVariability
Color composite thumbnail image of M33-013358.05J013358.05+304539.9M33-013358.05Warm-Hypergiant 16.85TableGraphVariability
Color composite thumbnail image of V-120530J013411.33+303628.0V-120530Warm-Hypergiant 18.43TableGraphVariability
Color composite thumbnail image of V-125093J013415.42+302816.4V-125093Warm-Hypergiant 17.32TableGraphVariability

By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory

Generated on 2021-11-06 16:53:54 UT-5