MULTICOLOR PHOTOMETRY OF THE M DWARF PROXIMA CEN.
MULTICOLOR PHOTOMETRY OF THE M DWARF PROXIMA CEN.
复制标题
M 矮星比邻星中心的多色测光。
DOI：
10.1086/129334
复制
发表时间：
1972
影响因子：
3.5
通讯作者：
D. W. Strecker
中科院分区：
文献类型：
--
作者：
J. Frogel;D. Kleinmann;W. Kunkel;E. Ney;D. W. Strecker
对半人马座比邻星在0.3-5之间的光度观测表明，该恒星的有效温度为2700K，测辐射光度为6.7>；c 1030ergs sec-1，半径为1.3×1010厘米，与Greenstein、Neugebauer和Becklin(1970)对主序列弱端的定标结果一致。关键词：光度学-M矮星-低主序
Photometric observations of Proxima Centauri between 0.3 and 5 show that this star has an effective temperature of 2700 K, a bolometric luminosity of 6.7 >c 1030 ergs sec-1, and a radius of 1.3 x 1010 cm, agreeing with the calibration of the faint end of the main sequence made by Greenstein, Neugebauer, and Becklin (1970). Key words: photometry - M dwarf star - lower main sequence