Clusters: age scales for stellar physics release_vc2wsjupbfbrzfb3ul6qrvz7gq

by David Barrado

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abstracts[] {'sha1': '0c1cf0fe5197bf0d0a202f0d6ca2d100fd391a4f', 'content': 'Ages are key to truly understand a large plethora of astrophysical phenomena.\nOn the other hand, stellar clusters are open windows to understand stellar\nevolution, specifically, the change with time and mass of different stellar\nproperties. As such, they are our laboratories where different theories can be\ntested, but without accurate ages, our knowledge would impaired. We revisit\nhere a large number of age-dating techniques and discuss their advantages and\ndraw-backs. In addition, a step-by step process is suggested in order to built\na coherent age scale ladder, minimizing the error budget and the sources of\nuncertainty.', 'mimetype': 'text/plain', 'lang': 'en'}
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language en
license_slug ARXIV-1.0
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release_date 2016-09-11
release_stage accepted
release_type article
release_year 2016
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title Clusters: age scales for stellar physics
version v2
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work_id ygdlfsxcuvbhrgyqyw2pvqrd4i
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arxiv.base_id 1606.09448
arxiv.categories ['astro-ph.SR']
arxiv.comments Stellar clusters: benchmarks of stellar physics and galactic evolution - EES2015, E. Moraux, Y. Lebreton, and C. Charbonnel (eds.) EAS Publications Series, 2016