DISCOVERY OF 5 PRE-MAIN-SEQUENCE BINARIES IN TAURUS

被引:56
作者
CHEN, WP
SIMON, M
LONGMORE, AJ
HOWELL, RR
BENSON, JA
机构
[1] ROYAL OBSERV,EDINBURGH EH9 3HJ,MIDLOTHIAN,SCOTLAND
[2] UNIV WYOMING,DEPT PHYS & ASTRON,LARAMIE,WY 82070
关键词
Clusters: associations; Occultations; Stars: binaries; Stars: pre-main-sequence;
D O I
10.1086/168908
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the progress of our infrared K band lunar occultation search for binaries among pre-main sequence stars. From the fall of 1986 to the fall of 1989, 13 objects have been observed, all in the Taurus star-forming region. Five new binaries have been discovered: DF Tau, DI Tau, FS Tau (Haro 6-5) A, FV Tau (Haro 6-8), and FW Tau, with projected separations ranging from 0″.01 to 0″.57. Including results reported previously, we have, to date, surveyed a total of 31 objects, 21 in Taurus and 10 in Ophiuchus, and have found nine double systems. The detected binary frequency (0.29) seems consistent with that of the solar-type main-sequence field stars.
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页码:224 / 230
页数:7
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