Characterising LMC Star Cluster NGC 2004.

التفاصيل البيبلوغرافية
العنوان: Characterising LMC Star Cluster NGC 2004.
المؤلفون: Nikolov, Grigor, Markov, Haralambi
المصدر: AIP Conference Proceedings; 2019, Vol. 2075 Issue 1, p090005-1-090005-6, 6p, 1 Chart, 3 Graphs
مصطلحات موضوعية: LARGE magellanic cloud, STAR clusters, ASTRONOMICAL observations, CLUSTER theory (Nuclear physics), STELLAR populations
الشركة/الكيان: HUBBLE Space Telescope (Spacecraft)
مستخلص: Hubble Space Telescope observations of NGC 2004, a cluster located in the Large Magellanic Cloud, have been used to derive an improved age estimate of the stellar population by means of isochrones fitting and synthetic cluster comparison. The cluster’s structural parameters have been calculated from a model based on number-density profiles, giving radius of the core 2.85 ± 0.46 parsecs. [ABSTRACT FROM AUTHOR]
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قاعدة البيانات: Complementary Index
الوصف
تدمد:0094243X
DOI:10.1063/1.5091219