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arXiv · 1504.03349

Witnessing the Emergence of a Carbon Star

L. Guzman-Ramirez·E. Lagadec·R. Wesson·A. A. Zijlstra·A. Muller·D. Jones·H. M. J. Boffin·G. C. Sloan·M. P. Redman·A. Smette·A. I. Karakas·Lars-Ake Nyman
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Abstract

During the late stages of their evolution, Sun-like stars bring the products of nuclear burning to the surface. Most of the carbon in the Universe is believed to originate from stars with masses up to a few solar masses. Although there is a chemical dichotomy between oxygen-rich and carbon-rich evolved stars, the dredge-up itself has never been directly observed. In the last three decades, however, a few stars have been shown to display both carbon- and oxygen-rich material in their circumstellar envelopes. Two models have been proposed to explain this dual chemistry: one postulates that a recent dredge-up of carbon produced by nucleosynthesis inside the star during the Asymptotic Giant Branch changed the surface chemistry of the star. The other model postulates that oxygen-rich material exists in stable keplerian rotation around the central star. The two models make contradictory, testable, predictions on the location of the oxygen-rich material, either located further from the star than the carbon-rich gas, or very close to the star in a stable disk. Using the Faint Object InfraRed CAmera (FORCAST) instrument on board the Stratospheric Observatory for Infrared Astronomy (SOFIA) Telescope, we obtained images of the carbon-rich planetary nebula (PN) BD+30 3639 which trace both carbon-rich polycyclic aromatic hydrocarbons (PAHs) and oxygen-rich silicate dust. With the superior spectral coverage of SOFIA, and using a 3D photoionisation and dust radiative transfer model we prove that the O-rich material is distributed in a shell in the outer parts of the nebula, while the C-rich material is located in the inner parts of the nebula. These observations combined with the model, suggest a recent change in stellar surface composition for the double chemistry in this object. This is evidence for dredge-up occurring ~1000yr ago.

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L. Guzman-Ramirez, E. Lagadec, R. Wesson, A. A. Zijlstra, A. Muller, D. Jones, H. M. J. Boffin, G. C. Sloan, M. P. Redman, A. Smette, A. I. Karakas, Lars-Ake Nyman. 2015-04-13. Witnessing the Emergence of a Carbon Star. https://doi.org/10.1093/mnrasl/slv055

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