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    Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/102058


    Title: The Pan-STARRS 1 discoveries of five new neptune trojans
    Authors: 葉永烜;Lin (林省文), Hsing Wen;Chen (陳英同), Ying-Tung;Holman, Matthew J.;Ip (葉永烜), Wing-Huen;Payne, M. J.;Lacerda, P.;Fraser, W. C.;Gerdes, D. W.;Bieryla, A.;Sie (謝宗富), Z.-F.;Chen (陳文屏), W.-P.;Burgett, W. S.;Denneau, L.;Jedicke, R.;Kaiser, N.;Magnier, E. A.;Tonry, J. L.;Wainscoat, R. J.;Waters, C.
    Contributors: 理學院天文研究所
    Keywords: Confidence;Inclination;Kuiper belt: general;Malware;minor planets, asteroids: general;Neptune;Origins;Physical properties;Pipelines;Simulation;surveys
    Date: 2016-11-01
    Issue Date: 2026-04-21 14:58:39 (UTC+8)
    Publisher: IOP Publishing Ltd.;The American Astronomical Society
    Abstract: 摘要: ABSTRACT In this work, we report the detection of seven Neptune Trojans (NTs) in the Pan-STARRS 1 (PS1) survey. Five of these are new discoveries, consisting of four L4 Trojans and one L5 Trojan. Our orbital simulations show that the L5 Trojan stably librates for only several million years. This suggests that the L5 Trojan must be of recent capture origin. On the other hand, all four new L4 Trojans stably occupy the 1:1 resonance with Neptune for more than 1 Gyr. They can, therefore, be of primordial origin. Our survey simulation results show that the inclination width of the NT population should be between 7° and 27° at >95% confidence, and most likely ∼11°. In this paper, we describe the PS1 survey, the Outer Solar System pipeline, the confirming observations, and the orbital/physical properties of the new NTs.
    其他題名: AJ
    其他題名: Astron. J
    出版者: The American Astronomical Society
    出版日期: 2016-11-01
    出處: The Astronomical journal, 2016-11, Vol.152 (5), p.147-147
    資源來源: Institute of Physics Journals
    版權: 2016. The American Astronomical Society. All rights reserved.
    識別號: ISSN: 0004-6256
    識別號: ISSN: 1538-3881
    識別號: EISSN: 1538-3881
    識別號: DOI: 10.3847/0004-6256/152/5/147
    Appears in Collections:[Graduate Institute of Astronomy] journal & Dissertation

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