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The age of 47 Tuc from self-consistent isochrone fits to colour–magnitude diagrams and the eclipsing member V69

Brogaard, K. and VandenBerg, D. A. and Bedin, L. R. and Milone, A. P. and Thygesen, A. O. and Grundahl, F. (2017) The age of 47 Tuc from self-consistent isochrone fits to colour–magnitude diagrams and the eclipsing member V69. Monthly Notices of the Royal Astronomical Society, 468 (1). pp. 645-661. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20170428-124454978

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Abstract

Our aim is to derive a self-consistent age, distance and composition for the globular cluster 47 Tucanae (47 Tuc; NGC104). First, we re-evaluate the reddening towards the cluster resulting in a nominal E(B − V) = 0.03 ± 0.01 as the best estimate. The Teff of the components of the eclipsing binary member V69 is found to be 5900 ± 72 K from both photometric and spectroscopic evidence. This yields a true distance modulus (m − M)0 = 13.21 ± 0.06(random) ±0.03(systematic) to 47 Tuc when combined with existing measurements of V69 radii and luminosity ratio. We then present a new completely self-consistent isochrone fitting method to ground-based and Hubble Space Telescope cluster colour–magnitude diagrams and the eclipsing binary member V69. The analysis suggests that the composition of V69, and by extension one of the populations of 47 Tuc, is given by [Fe/H] ∼ −0.70, [O/Fe] ∼ +0.60 and Y ∼ 0.250 on the solar abundance scale of Asplund, Grevesse & Sauval. However, this depends on the accuracy of the model Teff scale that is 50–75 K cooler than our best estimate but within measurement uncertainties. Our best estimate of the age of 47 Tuc is 11.8 Gyr, with firm (3σ) lower and upper limits of 10.4 and 13.4 Gyr, respectively, in satisfactory agreement with the age derived from the white dwarf cooling sequence if our determination of the distance modulus is adopted.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1093/mnras/stx378DOIArticle
https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stx378PublisherArticle
https://arxiv.org/abs/1702.03421arXivDiscussion Paper
ORCID:
AuthorORCID
Thygesen, A. O.0000-0002-4912-1183
Additional Information:© 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. Received 14 November 2016; revision received 07 February 2017; accepted 09 February 2017; published 14 February 2017. We wish to thank Luca Casagrande for useful discussions on interstellar reddening. We thank P. Stetson, J. Kaluzny and E. Garcia-Berro for quick and useful responses to inquiries related to this work. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (grant DNRF106). The research was supported by the ASTERISK project (ASTERoseismic Investigations with SONG and Kepler) funded by the European Research Council (grant agreement no.: 267864). KB acknowledges support from the Villum Foundation and the Carlsberg Foundation. A Discovery Grant from the Natural Sciences and Engineering Council of Canada supported the contribution to this project by DAV. APM acknowledges support by the Australian Research Council through the Discovery Early Career Researcher Awards DE150101816. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. The Digitized Sky Surveys were produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions.
Funders:
Funding AgencyGrant Number
Danish National Research FoundationDNRF106
European Research Council (ERC)267864
Villum FoundationUNSPECIFIED
Carlsberg FoundationUNSPECIFIED
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Australian Research CouncilDE150101816
NASANAS5-26555
NASANNX09AF08G
NASANAG W-2166
Subject Keywords:Binaries: eclipsing; Hertzsprung–Russell and colour–magnitude diagrams; Globular clusters: individual: 47 Tuc (NGC104)
Record Number:CaltechAUTHORS:20170428-124454978
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170428-124454978
Official Citation:K. Brogaard, D. A. VandenBerg, L. R. Bedin, A. P. Milone, A. Thygesen, F. Grundahl; The age of 47 Tuc from self-consistent isochrone fits to colour–magnitude diagrams and the eclipsing member V69. Mon Not R Astron Soc 2017; 468 (1): 645-661. doi: 10.1093/mnras/stx378
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:77059
Collection:CaltechAUTHORS
Deposited By: Melissa Ray
Deposited On:28 Apr 2017 20:14
Last Modified:21 Sep 2017 22:48

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