Witnessing the emergence of a carbon star

Lizette Guzman-Ramirez, Eric Lagadec, Roger Wesson, Albert Auke Zijlstra, A A Muller, David Ian Jones, Henri MJ Boffin, Gregory C Sloan, Matthew Peter Redman, Alain Smette, Amanda Irene Karakas, Lars-Ake Nyman

Research output: Contribution to journalArticleResearchpeer-review

11 Citations (Scopus)

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 disc. 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 BD +30° 3639 which trace both carbon-rich polycyclic aromatic hydrocarbons and oxygen-rich silicate dust. With the superior spectral coverage of SOFIA, and using a 3D photoionization 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 ∼103 yr ago.
Original languageEnglish
Article numberL1-L5
Pages (from-to)1 - 5
Number of pages5
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume451
Issue number1
DOIs
Publication statusPublished - 21 Jul 2015
Externally publishedYes

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