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    Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/101028


    Title: The stellar content of the young open cluster trumpler 37
    Authors: 陳文屏;Errmann, R.;Neuhäuser, R.;Marschall, L.;Torres, G.;Mugrauer, M.;Chen, W.P.;Hu, S.C.-L.;Briceno, C.;Chini, R.;Bukowiecki, Ł.;Dimitrov, D.P.;Kjurkchieva, D.;Jensen, E.L.N.;Cohen, D.H.;Wu, Z.-Y.;Pribulla, T.;Vaňko, M.;Krushevska, V.;Budaj, J.;Oasa, Y.;Pandey, A.K.;Fernandez, M.;Kellerer, A.;Marka, C.
    Contributors: 理學院天文研究所
    Keywords: Astronomy and Astrophysics;Astrophysics;Magnetic fields;open clusters and associations: individual (Trumpler 37);Space and Planetary Science;Spectrum analysis;Stars & galaxies
    Date: 2013-08-01
    Issue Date: 2026-04-21 14:21:37 (UTC+8)
    Publisher: Wiley-VCH Verlag;Berlin: WILEY-VCH Verlag
    Abstract: 摘要: AbstractWith an apparent cluster diameter of 1.5° and an age of 4 Myr, Trumpler 37 is an ideal target for photometric monitoring of young stars as well as for the search of planetary transits, eclipsing binaries and other sources of variability. The YETI consortium has monitored Trumpler 37 throughout 2010 and 2011 to obtain a comprehensive view of variable phenomena in this region. In this first paper we present the cluster properties and membership determination as derived from an extensive investigation of the literature. We also compared the coordinate list to some YETI images. For 1872 stars we found literature data. Among them 774 have high probability of being member and 125 a medium probability. Based on infrared data we re‐calculate a cluster extinction of 0.9–1.2 mag. We can confirm the age and distance to be 3–5 Myr and870 pc. Stellar masses are determined from theoretical models and the mass function is fitted with a power‐law index of α = 1.90 (0.1–0.4 M⊙) and α = 1.12 (1–10 M⊙). (© 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
    其他題名: Astron. Nachr
    出版者: Berlin: WILEY-VCH Verlag
    出版日期: 2013-08
    出處: Astronomische Nachrichten, 2013-08, Vol.334 (7), p.673-681
    資源來源: Wiley Online Library Journals
    版權: Copyright © 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim
    版權: Copyright © 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
    識別號: ISSN: 0004-6337
    識別號: EISSN: 1521-3994
    識別號: DOI: 10.1002/asna.201311890
    Appears in Collections:[Graduate Institute of Astronomy] journal & Dissertation

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