{ "id": "2010.02545", "version": "v1", "published": "2020-10-06T08:24:04.000Z", "updated": "2020-10-06T08:24:04.000Z", "title": "Rapid evolution of [WC] stars in the Magellanic Clouds", "authors": [ "Marcin Hajduk" ], "comment": "11 pages, 2 figures", "journal": "2020, A&A, 642, A71", "doi": "10.1051/0004-6361/202038049", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "We obtained new spectra of fourteen Magellanic Cloud planetary nebulae with the South African Large Telescope to determine heating rates of their central stars and to verify evolutionary models of post-asymptotic giant branch stars. We compared new spectra with observations made in previous years. Five planetary nebulae showed an increase in excitation over time. Four of their central stars exhibit [WC] features in their spectra, including three new detections. This raises the total number of [WC] central stars of PNe in the Magellanic Clouds to ten. We compared determined heating rates of the four [WC] central stars with the He-burning post-asymptotic giant branch evolutionary tracks and the remaining star with the H-burning tracks. Determined heating rates are consistent with the evolutionary models for both H and He-burning post-asymptotic giant branch stars. The central stars of the PNe that show the fastest increase of excitation are also the most luminous in the sample. This indicates that [WC] central stars in the Magellanic Clouds evolve faster than H-burning central stars, and they originate from more massive progenitors.", "revisions": [ { "version": "v1", "updated": "2020-10-06T08:24:04.000Z" } ], "analyses": { "keywords": [ "central stars", "post-asymptotic giant branch stars", "giant branch evolutionary tracks", "magellanic cloud planetary nebulae", "rapid evolution" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable" } } }