The mass–radius relationship for very low mass stars: four new discoveries from the HATSouth Survey

The mass–radius relationship for very low mass stars: four new discoveries from the HATSouth Survey
复制标题

DOI:
10.1093/mnras/stt2100
复制
发表时间:
2013-10
影响因子:
4.8
通讯作者:
G. Zhou;D. Bayliss;J. Hartman;J. Hartman;G. Bakos;G. Bakos;K. Penev;K. Penev;Z. Csubry;Z. Csubry;T. Tan;A. Jordán;L. Mancini;M. Rabus;R. Brahm;N. Espinoza;M. Mohler-Fischer;S. Ciceri;V. Suc;B. Cs'ak;T. Henning;Brian P. Schmidt
G. Zhou;D. Bayliss;J. Hartman;J. Hartman;G. Bakos;G. Bakos;K. Penev;K. Penev;Z. Csubry;Z. Csubry;T. Tan;A. Jordán;L. Mancini;M. Rabus;R. Brahm;N. Espinoza;M. Mohler-Fischer;S. Ciceri;V. Suc;B. Cs'ak;T. Henning;Brian P. Schmidt
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
G. Zhou;D. Bayliss;J. Hartman;J. Hartman;G. Bakos;G. Bakos;K. Penev;K. Penev;Z. Csubry;Z. Csubry;T. Tan;A. Jordán;L. Mancini;M. Rabus;R. Brahm;N. Espinoza;M. Mohler-Fischer;S. Ciceri;V. Suc;B. Cs'ak;T. Henning;Brian P. Schmidt

文献摘要

被引文献

相似文献

HATSouth项目的开发得到了国家科学基金会核磁共振赠款NSF/AST-0723074的资助,运作得到了美国宇航局赠款NNX09AB29G的支持,后续观测得到了国家科学基金会/AST-1108686赠款的部分支持。澳大利亚国立大学的工作得到了ARC桂冠奖学金基金FL0992131的支持。用ESO2.2m/FEROS测量仪在MPI保证时间内进行随访观察[P087.A9014(A),P088.A-9008(A),P089.A-9008(A)]。AJ感谢智利经济部Fondecyt项目1130857、基础CATA PFB06和千年科学倡议的支持(核心:P10-022-F,P07-021-F)。RB和NE得到CONICYT-PCHA/Doctorado National的支持,MR得到Fondecyt博士后奖学金3120097的支持。我们承认使用了由罗伯特·马丁·艾尔斯科学基金资助的AAVSO光度全天调查(APASS)和设在法国斯特拉斯堡CDS的SIMBAD数据库。MPG/ESO 2.2米望远镜的工作是由马克斯·普朗克天文台和欧洲南方天文台联合进行的。
Development of the HATSouth project was funded by NSF MRI grant NSF/AST-0723074, operations are supported by NASA grant NNX09AB29G and follow-up observations receive partial support from grant NSF/AST-1108686. Work at the Australian National University is supported by ARC Laureate Fellowship Grant FL0992131. Follow-up observations with the ESO 2.2 m/FEROS instrument were performed under MPI guaranteed time [P087.A9014(A), P088.A-9008(A), P089.A-9008(A)]. AJ acknowledges support from FONDECYT project 1130857, BASAL CATA PFB06 and the Millenium Science Initiative, Chilean Ministry of Economy (Nuclei: P10-022-F, P07-021-F). RB and NE are supported by CONICYT-PCHA/Doctorado Nacional and MR is supported by FONDECYT postdoctoral fellowship 3120097. We acknowledge the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund, and the SIMBAD data base, operated at CDS, Strasbourg, France. Operations at the MPG/ESO 2.2 m telescope are jointly performed by the Max Planck Gesellschaft and the European Southern Observatory.