容纳极高质量恒星的较小质量星团
太阳与恒星天体物理
2015-10-08 v1
摘要
我们呈现了年轻开放星团 VVV CL041 的首次物理表征。我们对星团主序恒星族群及一颗极高质量恒星候选体 WR62-2 进行了光谱观测。对我们的近红外光谱的 CMFGEN 建模表明，WR62-2 是一颗极亮 (10) 且大质量 () 的恒星。
引用
@article{arxiv.1510.01939,
title = {A not so massive cluster hosting a very massive star},
author = {S. Ramírez Alegría and A. -N. Chené and J. Borissova and R. Kurtev and C. Navarro and M. Kuhn and J. A. Carballo-Bello},
journal= {arXiv preprint arXiv:1510.01939},
year = {2015}
}
备注
1 page, 1 figure, to be published in the "International Workshop on Wolf-Rayet Stars conference proceedings" by Universit\"atsverlag Potsdam (editors: W.-R. Hamann, A. Sander, and H. Todt)