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NGC 6366 - 版本历史
2026-07-16T05:53:05Z
在这个wiki上该页的修订历史
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imported>迴廊彼端：調整內部連結
2025-04-27T05:36:26Z
<p>調整內部連結</p>
<p><b>新页面</b></p><div>{{Infobox globular cluster<br />
| name = NGC 6366<br />
| image = NGC 6366 HST 10775 R814B606.png<br />
| caption = 通過[[哈伯太空望遠鏡]]看到的NGC 6366<br />
| epoch = [[J2000]]<br />
| pronounce =<br />
| constellation = [[蛇夫座]]<br />
| class = XI<br />
| ra = {{RA|17|27|44.3}} <!-- or {{Deg2HMS|000.0000|sup=yes}} --><br />
| dec = {{DEC|-05|04|36}}<br />
| z = <!--{{Val||}}--><br />
| h_radial_v = {{Val|-122|0.5|u=km/s}}<br />
| gal_v = <!--{{Val|||u=km/s}}--><br />
| dist_pc = <!--{{Convert|000|+/-|00|kpc|kly|abbr=on|lk=on}}{{hub|0.73}}--><br />
| dist_ly = <!--{{Convert|000|+/-|00|kly|kpc|abbr=on|lk=on}}{{hub|0.73}}--><br />
| group_cluster = <br />
| type = XI<br />
| mass = <!-- In solar masses --> <!--{{Val|0|e=0}}--> <br />
| mass_light_ratio = <!-- In solar units --><br />
| size = <!-- In light years --><br />
| stars = <br />
|metal_fe== −0.60{{±|0.03}}<ref name=Puls2018>{{Citation|arxiv=1801.09968|year=2018|title=Chemical analysis of eight giant stars of the globular cluster NGC 6366|doi=10.1093/mnras/sty267 |last1=Puls |first1=Arthur A. |last2=Alves-Brito |first2=Alan |last3=Campos |first3=Fabíola |last4=Dias |first4=Bruno |last5=Barbuy |first5=Beatriz |journal=Monthly Notices of the Royal Astronomical Society |volume=476 |pages=690–704 |doi-access=free }}</ref><br />
| appmag_v = 9.5<br />
| absmag_v = -5.47<br />
| size_v = 13.0'<br />
| notes = <br />
| names = GCL 65<br />
| references = NASA/IPAC extragalactic datatbase, http://spider.seds.org/<br />
}}<br />
<br />
'''NGC 6366'''是在星座[[蛇夫座]]中的一個[[球狀星團]]。它是德國天文學家[[弗里德里希·奧古斯特·特奧多爾·溫尼克]]於1860年4月12日發現的，在[[夏普力-索耶集中度分類法]]中被歸類為「XI」<ref name=cseligman>{{Cite web|title=NGC 6366 (= GCL 65)|url=http://cseligman.com/text/atlas/ngc63a.htm#6366|website=cseligman|access-date=19 October 2015}}</ref>。它距離[[地球]]11,700[[光年]]<ref name="NASA/IPAC">{{Cite web|title=Object No. 1 - NGC 6366|url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+6366&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|website=NASA/IPAC extragalactic database|publisher=NASA/IPAC|access-date=19 October 2015}}</ref><ref name=Seds>{{Cite web|title=Revised NGC Data for NGC 6366|url=http://spider.seds.org/ngc/revngcic.cgi?NGC6366|website=Seds|access-date=19 October 2015}}</ref><ref name=Seds1>{{Cite web|title=NGC 6366|url=http://spider.seds.org/spider/MWGC/n6366.html|website=Seds|access-date=19 October 2015}}</ref><ref name=In-the-sky>{{Cite web|title=The globular cluster NGC 6366|url=https://in-the-sky.org/data/object.php?id=5117|website=In-the-sky|access-date=19 October 2015}}</ref>。<br />
<br />
NGC 6366的組成與 [[M71]]或[[NGC 6342]]相似<ref name=Johnson2016>{{Citation|arxiv=1606.08491|year=2016|title=The Chemical Composition of Red Giant Branch Stars in the Galactic Globular Clusters NGC 6342 and NGC 6366|doi=10.3847/0004-6256/152/1/21 |last1=Johnson |first1=Christian I. |last2=Caldwell |first2=Nelson |last3=Rich |first3=R. Michael |last4=Pilachowski |first4=Catherine A. |last5=Hsyu |first5=Tiffany |journal=The Astronomical Journal |volume=152 |issue=1 |page=21 |bibcode=2016AJ....152...21J |s2cid=19812549 |doi-access=free }}</ref>。對於一個球狀星團來說，它富含金屬，它的所有恆星似乎都是在同一個時代形成的<ref name=Puls2018/>。<br />
<br />
== 相關條目 ==<br />
* [[NGC天體列表 (6000-6999)]]<br />
* [[NGC天體列表]]<br />
<br />
== 參考資料 ==<br />
{{Reflist}}<br />
<br />
== 外部連結 ==<br />
* {{Commons category-inline}}<br />
<br />
[[Category:球狀星團]]<br />
[[Category:NGC天體|6366]]<br />
[[Category:蛇夫座]]<br />
[[Category:1860年發現的天體]]<br />
<br />
{{Star-cluster-stub}}</div>
imported>迴廊彼端