First Millimeter Detection of the Disk around a Young, Isolated, Planetary-mass Object | |
Bayo, Amelia; Joergens, Viki; Liu, Yao; Brauer, Robert; Olofsson, Johan; Arancibia, Javier; Pinilla, Paola; Wolf, Sebastian; Ruge, Jan Philipp; Henning, Thomas | |
刊名 | ASTROPHYSICAL JOURNAL LETTERS
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2017 | |
卷号 | 841期号:1页码:L11- |
英文摘要 | OTS44 is one of only four free-floating planets known to have a disk. We have previously shown that it is the coolest and least massive known free-floating planet (similar to 12 M-Jup) with a substantial disk that is actively accreting. We have obtained Band 6 (233 GHz) ALMA continuum data of this very young disk-bearing object. The data show a clear unresolved detection of the source. We obtained disk-mass estimates via empirical correlations derived for young, higher-mass, central (substellar) objects. The range of values obtained are between 0.07 and 0.63 M-circle plus (dust masses). We compare the properties of this unique disk with those recently reported around higher-mass (brown dwarfs) young objects in order to infer constraints on its mechanism of formation. While extreme assumptions on dust temperature yield disk-mass values that could slightly diverge from the general trends found for more massive brown dwarfs, a range of sensible values provide disk masses compatible with a unique scaling relation between M-dust and M* through the substellar domain down to planetary masses. |
语种 | 英语 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/17371] ![]() |
专题 | 中国科学院紫金山天文台 |
推荐引用方式 GB/T 7714 | Bayo, Amelia,Joergens, Viki,Liu, Yao,et al. First Millimeter Detection of the Disk around a Young, Isolated, Planetary-mass Object[J]. ASTROPHYSICAL JOURNAL LETTERS,2017,841(1):L11-. |
APA | Bayo, Amelia.,Joergens, Viki.,Liu, Yao.,Brauer, Robert.,Olofsson, Johan.,...&Chauvin, Gael.(2017).First Millimeter Detection of the Disk around a Young, Isolated, Planetary-mass Object.ASTROPHYSICAL JOURNAL LETTERS,841(1),L11-. |
MLA | Bayo, Amelia,et al."First Millimeter Detection of the Disk around a Young, Isolated, Planetary-mass Object".ASTROPHYSICAL JOURNAL LETTERS 841.1(2017):L11-. |
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