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{{Infobox nebula
| name = NGC 6072
| image = File:NGC 6072.jpg
| caption = NGC 6072的[[史匹哲太空望遠鏡]]的NGC 6072影像
| credit = 
| type = 行星狀
| type2 = 
| epoch = [[J2000]]
| subtype =
| class =
| ra = {{RA|16|12|58.363}}<ref name=GaiaDR2/>
| dec = {{DEC|-36|13|47.40}}<ref name=GaiaDR2/>
| dist_ly = {{cvt|939|pc|ly|order=flip|lk=on}}<ref name=GaiaDR2/> {{cvt|1017|pc|ly|order=flip|abbr=off}}<ref name=Stanghellini_et_al_2008/>
| dist_pc =
| dist_z =
| appmag_v = 14<ref name="SEDS"/>
| appdia = 
| size_v = {{val|70|ul=arcsecond}}<ref name=Stanghellini_et_al_2008/>
| constellation = [[天蠍座]]
| radius_ly =
| radius_pc =
| dimensions =
| absmag_v =
| notes =
| names = {{odlist | NGC=6072 | PK=342+10 1| PN=Sa 2-134 | IRAS=F16097-3606 | SCM=107 }}<ref name=SIMBAD/>
}}

'''NGC 6072'''是位於[[天蠍座]]南部的一個[[行星狀星雲]]。它的動態年齡為104年。因為它有非常强的CN（[[氰化物]]）[[譜線]]，它的[[星周包層]]可能富含[[碳]]。在富含[[氧]]的AGB（[[漸近巨星分支]]）星周包層中通常無法檢測到CN光譜線。NGC 6072還顯示了H2（[[氫]]） [[發射光譜|發射]]和強烈的CO（[[一氧化碳]]）發射，這些發射已被繪製出來，顯示[[電磁場|雙極]]和一些高[[速度]]的氣體。這個[[行星狀星雲]]的[[演化]]很可能是由[[光分解作用|光解離]]和[[離子]]/[[自由基]][[分子]]反應主導的。休克[[化學反應]] 也可能很重要。

分析「[[蓋亞任務]]」的數據表明中心恆星是 [[聯星|聯星系統]]<ref name=Chornay_et_al_2021/>。

== 參考文獻 ==
{{reflist|refs=

<ref name=GaiaDR2>{{Cite Gaia DR2 | 2423493369021649920 }}</ref>

<ref name=SIMBAD>{{cite simbad
| title=NGC 6072 | access-date=2022-01-01 }}</ref>

<ref name=Stanghellini_et_al_2008>{{cite journal
| title=The Magellanic Cloud Calibration of the Galactic Planetary Nebula Distance Scale
| url=https://archive.org/details/sim_astrophysical-journal_2008-12-10_689_1/page/193
| display-authors=1 | last1=Stanghellini | first1=L.
| last2=Shaw | first2=RA. | last3=Villaver | first3=E.
| journal=The Astrophysical Journal
| volume=689 | issue=1 | pages=194–202 | year=2008
| doi=10.1086/592395 | bibcode=2008ApJ...689..194S
| arxiv=0807.1129 | s2cid=119257242 }}</ref>

<ref name="SEDS">{{cite web
| title=Students for the Exploration and Development of Space
| work=Results for NGC 6072
| url=http://seds.org/~spider/ngc/ngc.cgi?NGC6072
| archive-url=https://archive.today/20121228120238/http://seds.org/~spider/ngc/ngc.cgi?NGC6072
| url-status=dead
| archive-date=December 28, 2012
| access-date=2009-03-21
}}</ref>

<ref name=Chornay_et_al_2021>{{cite journal
| title=Towards a more complete sample of binary central stars of planetary nebulae with Gaia
| last1=Chornay | first1=N. | last2=Walton | first2=N. A.
| last3=Jones | first3=D. | last4=Boffin | first4=H. M. J.
| last5=Rejkuba | first5=M. | last6=Wesson | first6=R.
| display-authors=1 | journal=Astronomy & Astrophysics
| volume=648 | pages=A95 | year=2021
| arxiv=2101.01800 | bibcode=2021A&A...648A..95C
| doi=10.1051/0004-6361/202140288 | s2cid=230770301 }}</ref>

}}

== 外部連結 ==
* {{commons category-inline}}

{{Ngc65}}
{{天蝎座}}

[[Category:行星狀星雲]]
[[Category:NGC天體|6072]]
[[Category:天蠍座]]

{{nebula-stub}}

NGC 6072 - 版本历史

imported>InternetArchiveBot：​Add 1 book for verifiability (20251017sim)) #IABot (v2.0.9.5) (GreenC bot

imported>InternetArchiveBot：Add 1 book for verifiability (20251017sim)) #IABot (v2.0.9.5) (GreenC bot