红巨星分支尖端
天体物理学
2007-11-14 v1
摘要
我综述了红巨星分支尖端作为标准烛光在光学和近红外波段的最新校准结果。在考虑所有不确定性的情况下，不同且独立的经验校准之间的一致性相当好。还讨论了将该校准扩展到 SDSS 测光波段（i, z）的可能性。
引用
@article{arxiv.0711.2016,
title = {The Tip of the Red Giant Branch},
author = {M. Bellazzini},
journal= {arXiv preprint arXiv:0711.2016},
year = {2007}
}
备注
8 pages, 6 greyscale figures. Invited review. Proceedings of the workshop "XXI Century challenges for stellar evolution", held in Cefalu' (Sicily, Italy), August 29 - September 2, 2007; S. Cassisi and M. Salaris Eds. To be published in Mem. SAIt Vol. 79 No. 2