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High-Mass Triple Systems: The Classical Cepheid Y Carinae*

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© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Nancy Remage Evans et al 2005 AJ 130 789 DOI 10.1086/430458

1538-3881/130/2/789

Abstract

We have obtained a Hubble Space Telescope STIS ultraviolet high-dispersion echelle-mode spectrum of the binary companion of the double-mode classical Cepheid Y Car. The velocity measured for the hot companion from this spectrum is very different from reasonable predictions for binary motion, implying that the companion is itself a short-period binary. The measured velocity changed by 7 km s-1 during the 4 days between two segments of the observation, confirming this interpretation. We summarize "binary" Cepheids that are in fact members of a triple system and find that at least 44% are triples. The summary of information on Cepheids with orbits makes it likely that the fraction is underestimated.

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Footnotes

  • Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc.

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10.1086/430458