预测Kepler观测的太阳型恒星中振荡的可探测性
太阳与恒星天体物理
2015-05-27 v1
摘要
太阳型恒星的星震学在NASA Kepler任务的系外行星计划中发挥着重要作用。地震数据使得对恒星性质的精确且准确的推断成为可能，从而能够对系外行星系统施加非常严格的约束。在此，我们概述了如何利用对温度和半径的粗略估计以及Kepler视星等，来估计任何给定Kepler目标中类太阳振荡的可探测性。
引用
@article{arxiv.1103.0702,
title = {Predicting the detectability of oscillations in solar-type stars observed by Kepler},
author = {W. J. Chaplin and H. Kjeldsen and T. R. Bedding and J. Christensen-Dalsgaard and R. L. Gilliland and S. D. Kawaler and T. Appourchaux and Y. Elsworth and R. A. Garcia and G. Houdek and C. Karoff and T. S. Metcalfe and J. Molenda-Zakowicz and M. J. P. F. G. Monteiro and M. J. Thompson and G. A. Verner and N. Batalha and W. J. Borucki and T. M. Brown and S. T. Bryson and J. L. Christiansen and B. D. Clarke and J. M. Jenkins and T. C. Klaus and D. Koch and D. An and J. Ballot and S. Basu and O. Benomar and A. Bonanno and A. -M. Broomhall and T. L. Campante and E. Corsaro and O. L. Creevey and L. Esch and N. Gai and P. Gaulme and S. J. Hale and R. Handberg and S. Hekker and D. Huber and S. Mathur and B. Mosser and R. New and M. H. Pinsonneault and D. Pricopi and P. -O. Quirion and C. Regulo and I. W. Roxburgh and D. Salabert and D. Stello and M. D. Suran},
journal= {arXiv preprint arXiv:1103.0702},
year = {2015}
}
备注
21 pages, 6 figures, accepted for publication Astrophysical Journal