Separating the subdwarf populations may shed light on their formation history and give unique insights into the atmospheric processes that are thought to be responsible for their abundance diversity. Such a task requires complex and time consuming spectral analyses, which we started to tailor to our objectives a year ago. Here we report the updates that have been made over the past year and will be the standard method in SD1000.
@article{arxiv.1308.0260,
title = {SD1000 Collaboration: Hunting down the subdwarf populations},
author = {Peter Nemeth and Roy Østensen and Joris Vos and Adela Kawka and Stephane Vennes},
journal= {arXiv preprint arXiv:1308.0260},
year = {2013}
}
Comments
8 pages and 3 figures; to be published in the proceedings of the Sixth Meeting on Hot Subdwarf Stars and Related Objects