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Radiative levitation: a likely explanation for pulsations in the unique hot O subdwarf star SDSS J160043.6+074802.9

Fontaine, G. and Brassard, P. and Green, E. M. and Chayer, P. and Charpinet, S. and Andersen, M. and Portouw, J. (2008) Radiative levitation: a likely explanation for pulsations in the unique hot O subdwarf star SDSS J160043.6+074802.9. Astronomy and Astrophysics, 486 (3). L39-L42. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:FONaanda08

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Abstract

Context. SDSS J160043.6+074802.9 (J1600+0748 for short) is the only hot sdO star for which unambiguous multiperiodic luminosity variations have been reported so far. These rapid variations, with periods in the range from ~60 s to ~120 s, are best qualitatively explained in terms of pulsational instabilities, but the exact nature of the driving mechanism has remained a puzzle. Aims. Our primary goal is to examine quantitatively how pulsation modes can be excited in an object such as J1600+0748. Given the failure of uniform-metallicity models as well documented in the recent Ph.D. thesis of C. Rodríguez-López, we consider the effects of radiative levitation on iron as a means to boost the efficiency of the opacity-driving mechanism in models of J1600+0748. Methods. We combine high sensitivity time-averaged optical spectroscopy and full nonadiabatic calculations to carry out our study. In the first instance, this is used to estimate the location of J1600+0748 in the log $g-T_{\rm eff}$ plane. Given this essential input, we pulsate stellar models consistent with these atmospheric parameters. We construct both uniform-metallicity models and structures in which the iron abundance is specified by the condition of diffusive equilibrium between gravitational settling and radiative levitation. Results. On the basis of NTLE H/He synthetic spectra, we find that the target star has the following atmospheric parameters: log g = 5.93 $\pm$ 0.11, $T_{\rm eff}$ = 71 070 $\pm$ 2725 K, and log N(He)/N(H) = -0.85 $\pm$ 0.08. This takes into account our deconvolution of the spectrum of J1600+0748 as it is polluted by the light of a main sequence companion. We confirm that uniform-metallicity stellar models with Z in the range from 0.02 to 0.10 cannot excite pulsation modes of the kind observed. On the other hand, we find that the inclusion of radiative levitation, as we implemented it, leads to pulsational instabilities in a period range that overlaps with, although it is narrower than, the observed range in J1600+0748. The excited modes correspond to low-order, low-degree p-modes. Conclusions. We infer that radiative levitation is a likely essential ingredient in the excitation physics at work in J1600+0748.


Item Type:Article
Related URLs:
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http://dx.doi.org/10.1051/0004-6361:200810173DOIUNSPECIFIED
Additional Information:© ESO 2008. Article published by EDP Sciences.
Subject Keywords:stars: oscillations -- stars: subdwarfs -- stars: individual: SDSS J160043.6+074802.9
Issue or Number:3
Record Number:CaltechAUTHORS:FONaanda08
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:FONaanda08
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:12744
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:22 Dec 2008 18:44
Last Modified:03 Oct 2019 00:31

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