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Photometric Properties of Peculiar Red Giants

  • Conference paper
Cool Stars with Excesses of Heavy Elements

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 114))

Abstract

Four quite different kinds of information are commonly obtained through photometric observations: (1) magnitudes and colors on various systems; (2) energy distributions, leading to estimates of effective temperature, tests of model atmospheres, and the detection of companions or circumstellar shells; (3) spectroscopic data from narrow-band photometry of strong spectral features; and (4) light curves of variable stars. The photometric properties of the peculiar red giants — the cool carbon and S-type stars, and the warmer R-type carbon stars, CH stars, barium stars, and related objects — are reviewed with emphasis on what can be learned from each of these kinds of photometric data.

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  1. Astronomy Department, Ohio State University, Columbus, OH, 43210, USA

    Robert F. Wing

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  1. Strasbourg Observatory, Strasbourg, France

    Mercedes Jaschek

  2. Perkins Observatory, Delaware, Ohio, USA

    Philip C. Keenan

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Wing, R.F. (1985). Photometric Properties of Peculiar Red Giants. In: Jaschek, M., Keenan, P.C. (eds) Cool Stars with Excesses of Heavy Elements. Astrophysics and Space Science Library, vol 114. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5325-3_10

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  • DOI: https://doi.org/10.1007/978-94-009-5325-3_10

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