查看“︁NGC 1711”︁的源代码

{{NGCInfoBox|NGCID=NGC 1711|發現者=詹姆士·丹露帕|發現日期=1826年8月3日|其他編號=ESO 56-SC10|曆元=J2000.0|赤經=4時50分36.2秒
|赤緯=-69°59'8"|星座=山案座|星體=疏散星团|星等=10.1|表面亮度=|藍等=}}

'''NGC 1711'''，又記作'''ESO 56-SC10'''，是[[山案座]]的[[疏散星团]]，位處[[大麦哲伦星系]]之中，1826年由[[詹姆士·丹露帕]]發現。[[約翰·德雷耳]]將其列入原版[[NGC天體表|天體新總表]]（{{lang|en|NGC}}），形容為「球狀星團，明亮，小，不規則圓形，可明確分辨，明顯由14等恆星構成」。<ref name=":0222222">{{Cite web|language=en|url=http://cseligman.com/text/atlas/ngc17.htm|title=New General Catalog Objects: NGC 1700 - 1749|first=Courtney|last=Seligman|website=cseligman.com|date=|publisher=|access-date=2022-03-10|archive-date=2018-10-13|archive-url=https://web.archive.org/web/20181013192243/http://cseligman.com/text/atlas/ngc17.htm}}</ref>

星團年齡約四千六百萬年，[[金屬豐度]]為太陽的52 %。<ref>{{cite journal|url =http://adsabs.harvard.edu/abs/2019PASP..131b4101A|first1 =Andrea V.|last1= Ahumada|first2 = Luis R. |last2 = Vega-Neme|first3 =  Juan J. |last3= Clariá|first4 = Javier H.|last4= Minniti|title =Spectroscopic Fundamental Parameters of 16 Young Large Magellanic Cloud Star Clusters|date =2019-02-01|journal =Publications of the Astronomical Society of the Pacific|volume =131|issue = 996 |page = 024101|issn=0004-6280|doi=10.1088/1538-3873/aae660|language = en}}</ref>星團內，恆星的質量分佈由
:<math>\frac{\mathrm d N}{\mathrm d \ln m }\propto m^{\alpha}</math>
描述，其中<math>m</math>是質量，<math>N</math>是恆星數，指數<math>\alpha\approx -1.72</math>。<ref>{{cite journal |url =http://adsabs.harvard.edu/abs/2020ApJ...895...66M|first1 =Deepakshi |last1 = Madaan|first2 = Sophia|last2 = Lianou|first3 = Shantanu|last3 =  Basu|title =Using the Modified Lognormal Power-law Distribution to Model the Mass Function of NGC 1711|date =2020-05-01|journal =The Astrophysical Journal|volume =895|page =66|issn=0004-637X|doi=10.3847/1538-4357/ab88a6|language = en}}</ref>

== 參考文獻 ==
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{{NGCReference|1711}}