IAU GA SpS 5 II 总结：恒星与星风参数
太阳与恒星天体物理
2012-10-17 v1
摘要
红外观测设施的发展揭示了银河系内外遮蔽环境中存在的大量大质量恒星。因此，为了充分利用近红外和中红外available 的大量观测数据，必须通过红外诊断来确定它们的恒星和星风性质。然而，这项任务充满挑战。本次会议 addressed 了一些遇到的问题，并展示了大质量恒星红外研究的局限性与成功之处。
引用
@article{arxiv.1210.4280,
title = {Summary of IAU GA SpS 5 II: Stellar and Wind Parameters},
author = {F. Martins and M. Bergemann and J. M. Bestenlehner and P. A. Crowther and W. R. Hamann and F. Najarro and M. F. Nieva and N. Przybilla and J. Freimanis and W. Hou and L. Kaper and C. -D. Lee},
journal= {arXiv preprint arXiv:1210.4280},
year = {2012}
}
备注
10 pages, to be published in Highlights of Astronomy vol 16, 3rd part of the proceedings of special session #5 'IR view of massive stars' (ed. Y. Naze), a session which took place during the IAU general assembly 2012 ; see also http://www.gaphe.ulg.ac.be/IAU_XXVIII/prg.html