Solar-like oscillations in a metal-poor globular cluster with the HST

Abstract

We present analyses of variability in the red giant stars in the metal-poor globular cluster NGC6397, based on data obtained with the Hubble Space Telescope. We use an non-standard data reduction approach to turn a 23-day observing run originally aimed at imaging the white dwarf population, into time-series photometry of the cluster's highly saturated red giant stars. With this technique we obtain noise levels in the final power spectra down to 50 parts per million, which allows us to search for low amplitude solar-like oscillations. We compare the observed excess power seen in the power spectra with estimates of the typical frequency range, frequency spacing and amplitude from scaling the solar oscillations. We see evidence that the detected variability is consistent with solar-like oscillations in at least one and perhaps up to four stars. With metallicities two orders of magnitude lower than of the Sun, these stars present so far the best evidence of solar-like oscillations in such a low metallicity environment.

7 pages, 6 figures, accepted by ApJ

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Cited by in corpus (6)

• A Giant Planet Around a Metal-poor Star of Extragalactic Origin
• Integrated Mass Loss of Evolved Stars in M4 using Asteroseismology
• Asteroseismic Fingerprints of Stellar Mergers
• Indirect Probes of Dark Matter and Globular Cluster Properties From Dark Matter Annihilation within the Coolest White Dwarfs
• Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE - Constellation
• An observer's view on the future of asteroseismology