A candidate protoplanet in the Taurus star-forming region

被引:37
|
作者
Terebey, S
Van Buren, D
Padgett, DL
Hancock, T
Brundage, M
机构
[1] Extrasolar Res Corp, Pasadena, CA 91101 USA
[2] CALTECH, Jet Prop Lab, IPAC 100 22, Pasadena, CA 91125 USA
来源
ASTROPHYSICAL JOURNAL | 1998年 / 507卷 / 01期
关键词
binaries : general; circumstellar matter; infrared : stars; planetary systems; stars : formation; stars : individual (TMR-1);
D O I
10.1086/311671
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Hubble Space Telescope/Near-Infrared Camera and Multiobject Spectrometer images of the class I protostar TMR-I (IRAS 04361+2547) reveal a faint companion with 10." 0 = 1400 AU projected separation. The central protostar is itself resolved as a close binary with 0." 31 = 42 AU separation, surrounded by circumstellar reflection nebulosity. A long narrow filament seems to connect the protobinary to the faint companion TMR-1C, suggesting a physical association. If the sources are physically related, then we hypothesize that TMR-1C has been ejected by the protobinary. If TMR-1C has the same age and distance as the protobinary, then current models indicate that its flux is consistent with a young giant planet of several Jovian masses.
引用
收藏
页码:L71 / L74
页数:4
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