A study of the rapid rotator ζ Aql: differential surface rotation?
Article
Howarth, Ian D., Bailey, Jeremy, Cotton, Daniel V. and Kedziora-Chudczer, Lucyna. 2023. "A study of the rapid rotator ζ Aql: differential surface rotation?" Monthly Notices of the Royal Astronomical Society. 520 (1), pp. 1193-1209. https://doi.org/10.1093/mnras/stad149
Article Title | A study of the rapid rotator ζ Aql: differential surface rotation? |
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ERA Journal ID | 1074 |
Article Category | Article |
Authors | Howarth, Ian D., Bailey, Jeremy, Cotton, Daniel V. and Kedziora-Chudczer, Lucyna |
Journal Title | Monthly Notices of the Royal Astronomical Society |
Journal Citation | 520 (1), pp. 1193-1209 |
Number of Pages | 17 |
Year | 2023 |
Publisher | Oxford University Press |
Place of Publication | United Kingdom |
ISSN | 0035-8711 |
1365-2966 | |
Digital Object Identifier (DOI) | https://doi.org/10.1093/mnras/stad149 |
Web Address (URL) | https://academic.oup.com/mnras/article/520/1/1193/6987700 |
Abstract | We report new, extremely precise photopolarimetry of the rapidly-rotating A0 main-sequence star ? Aql, covering the wavelength range ?400–900 nm, which reveals a rotationally-induced signal. We model the polarimetry, together with the flux distribution and line profiles, in the framework of Roche geometry with ?-model gravity darkening, to establish the stellar parameters. An additional constraint is provided by TESS photometry, which shows variability with a period, Pphot, of 11.1 h. Modelling based on solid-body surface rotation gives rotation periods, Prot, that are in only marginal agreement with this value. We compute new ESTER stellar-structure models to predict horizontal surface-velocity fields, which depart from solid-body rotation at only the ?2 per cent level (consistent with a reasonably strong empirical upper limit on differential rotation derived from the line-profile analysis). These models bring the equatorial rotation period, Prot(e), into agreement with Pphot, without requiring any ‘fine tuning’ (for the Gaia parallax). We confirm that surface abundances are significantly subsolar ([M/H] ? ?0.5). The star’s basic parameters are established with reasonably good precision: M = 2.53 ± 0.16 M?, log (L/L?) = 1.72± 0.02, Rp = 2.21 ± 0.02 R?, Teff = 9693 ± 50 K, i = 85+?75?, and ?e/?c = 0.95 ± 0.02. Comparison with single-star solar-abundance stellar-evolution models incorporating rotational effects shows excellent agreement (but somewhat poorer agreement for models at [M/H] ? ?0.4). |
Keywords | polarization; stars: fundamental parameters; stars: individual : ζ Aql; stars: rotation |
ANZSRC Field of Research 2020 | 510109. Stellar astronomy and planetary systems |
Public Notes | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2023 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Byline Affiliations | University College London, United Kingdom |
University of New South Wales | |
Monterey Institute for Research in Astronomy, United States | |
Western Sydney University | |
Centre for Astrophysics |
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https://research.usq.edu.au/item/z25z4/a-study-of-the-rapid-rotator-aql-differential-surface-rotation
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