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{{Infobox nebula
| name = NGC 6153
| image = A nitrogen-rich nebula.jpg
| image_scale = 1.4
| alt =
| caption = [[哈伯太空望遠鏡|HST]]的NGC 6153影像<ref name=HST/>
| credit = 
| type = 行星狀
| type2 = 
| epoch = [[J2000]]
| subtype =
| class = II<ref name=VizieR/>
| ra = {{RA|16|31|30.57}}<ref name=EDR3/>
| dec = {{DEC|−40|15|12.6}}<ref name=EDR3/>
| dist_ly = {{cvt|1.499|±|0.300|kpc|ly|disp=output number only}}<ref name=Stanghellini_Haywood_2010/>
| dist_pc =
| dist_z =
| appmag_v = 10.6<ref name=Griffiths_2012/>
| appdia = {{val|30|ul=arcsecond}}<ref name=Griffiths_2012/>
| size_v =
| constellation = [[天蠍座]]
| radius_ly =
| radius_pc =
| dimensions =
| absmag_v =
| notes =
| names =
}}

'''NGC 6153'''是位於南天[[星座]][[天蠍座]]的一個行星狀星雲。英國天文學家[[羅夫·科普蘭]]在1883年發現了它<ref name=cseligman/>。這個星雲用孔徑小到 {{cvt|80|mm|in}}就能看見，但豐富的[[銀河系]]背景可能會使其難以找到。它的[[視星等]]為10.6，[[角直徑]]跨度為{{val|30|ul=arcsecond}}<ref name=Griffiths_2012/>。

這是一個大致對稱的雙極星雲，膨脹速度為{{val|12.7|to|17.3|u=km/s}}<ref name=Pottasch_et_al_1986/>。它包括一些結、細絲，可能還有雙層殼結構<ref name=Anandarao_Banerjee_1988/>。NGC 6153屬於Peimbert I型，表明它富含氦和氮，其前身是一顆[[薄盤]]恆星<ref name=Quireza_et_al_2007/>。1986年對[[恆星光譜]]的分析表明，這是一個不尋常的星雲。星雲中幾乎所有的元素，尤其是氮、氖、硫和氬，都過量了。在某些情况下，其豐度高於其它任何星雲<ref name=Pottasch_et_al_1986/>。有人提出，這種差異是由於星雲中的冷、富含金屬、缺氫的結構造成的<ref name=Yuan_et_al_2011/>。

對「蓋亞」數據的分析表明，中心恆星可能是一個[[聯星|聯星系統]]<ref name=Chornay_et_al_2021/>。聯星系統可以解釋豐度差異<ref name=McNabb_et_al_2016/>。在冷卻軌跡上，白矮星可能會經歷最後的[[漸近巨星支#後期熱脈衝|熱脈衝]]，導致恆星膨脹成一顆燃燒氦氣的巨星，其演化軌跡與早期恆星幾乎相同<ref name=Iben_et_al_1983/>。

== 參考文獻 ==
{{reflist|refs=

<ref name="VizieR">{{cite web
| work=VizieR Catalogue Database
| title=Results for NGC 6153
| url=http://vizier.cfa.harvard.edu/viz-bin/VizieR-5?-out.all=1&-source=VII/1B&-c=NGC+6139,rm=5.0
| access-date=2013-09-06
| archive-date=2016-03-04
| archive-url=https://web.archive.org/web/20160304111231/http://vizier.cfa.harvard.edu/viz-bin/VizieR-5?-out.all=1&-source=VII/1B&-c=NGC+6139,rm=5.0
| dead-url=no
}}</ref>

<ref name=cseligman>{{cite web
| title=New General Catalogue objects: NGC 6150 - 6199
| last=Seligman
| first=Courtney
| website=cseligman.com
| url=https://cseligman.com/text/atlas/ngc61a.htm#6153
| access-date=27 September 2019
| archive-date=2018-10-13
| archive-url=https://web.archive.org/web/20181013184244/http://cseligman.com/text/atlas/ngc61a.htm#6153
| dead-url=no
}}</ref>

<ref name=EDR3>{{Cite Gaia EDR3|6017034570775817984}}</ref>

<ref name=HST>{{cite web
| title=A nitrogen-rich nebula
| website=EAS/Hubble
| url=https://esahubble.org/images/potw1525a/
| access-date=14 January 2025
| archive-date=2018-09-11
| archive-url=https://web.archive.org/web/20180911200408/https://www.spacetelescope.org/images/potw1525a/
| dead-url=no
}}</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
| doi=10.1051/0004-6361/202140288 | arxiv=2101.01800
| bibcode=2021A&A...648A..95C | s2cid=230770301 }}</ref>

<ref name=Stanghellini_Haywood_2010>{{cite journal
| title=The Galactic Structure and Chemical Evolution Traced by the Population of Planetary Nebulae
| last1=Stanghellini | first1=Letizia | last2=Haywood | first2=Misha
| journal=The Astrophysical Journal
| volume=714 | issue=2 | pages=1096–1107 | date=May 2010
| doi=10.1088/0004-637X/714/2/1096 | arxiv=1003.0759
| bibcode=2010ApJ...714.1096S }}</ref>

<ref name=Griffiths_2012>{{cite book
| title=Planetary Nebulae and How to Observe Them
| first=Martin | last=Griffiths | year=2012
| page=253 | isbn=9781461417828
| publisher=Springer New York
| url=https://books.google.com/books?id=gsI1S_KVDxoC&pg=PA253 }}</ref>

<ref name=Quireza_et_al_2007>{{cite journal
| title=Bayesian posterior classification of planetary nebulae according to the Peimbert types
| display-authors=1 | last1=Quireza | first1=C.
| last2=Rocha-Pinto | first2=H. J. | last3=Maciel | first3=W. J.
| journal=Astronomy and Astrophysics
| volume=475 | issue=1 | date=November 2007 | pages=217–231
| doi=10.1051/0004-6361:20078087 | arxiv=0709.0711
| bibcode=2007A&A...475..217Q }}</ref>

<ref name=Pottasch_et_al_1986>{{cite journal
| title=Abundances in the planetary nebula NGC 6153
| url=https://archive.org/details/sim_astronomy-and-astrophysics_1986-02_155_2/page/396
| display-authors=1 | last1=Pottasch | first1=S. R.
| last2=Dennefeld | first2=M. | last3=Mo | first3=J.
| journal=Astronomy and Astrophysics
| volume=155 | pages=397–401 | date=February 1986
| bibcode=1986A&A...155..397P }}</ref>

<ref name=Anandarao_Banerjee_1988>{{cite journal
| title=High resolution observations of the planetary nebulae NGC 6153 and IC 4593
| url=https://archive.org/details/sim_astronomy-and-astrophysics_1988-08_202_1-2/page/n252
| last1=Anandarao | first1=B. G. | last2=Banerjee | first2=D. P. K.
| journal=Astronomy and Astrophysics
| volume=202 | pages=215–218 | date=August 1988
| bibcode=1988A&A...202..215A }}</ref>

<ref name=Yuan_et_al_2011>{{cite journal
| title=Three-dimensional chemically homogeneous and bi-abundance photoionization models of the 'super-metal-rich' planetary nebula NGC 6153
| last1=Yuan | first1=H. -B. | last2=Liu | first2=X. -W.
| last3=Péquignot | first3=D. | last4=Rubin | first4=R. H.
| last5=Ercolano | first5=B. | last6=Zhang | first6=Y.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=411 | issue=2 | pages=1035–1052 | date=February 2011
| doi=10.1111/j.1365-2966.2010.17732.x | doi-access=free | arxiv=1009.6148
| bibcode=2011MNRAS.411.1035Y | display-authors=1 }}</ref>

<ref name=McNabb_et_al_2016>{{cite journal
| title=Very Large Telescope deep echelle spectroscopy of Galactic planetary nebulae NGC 6153, M 1-42 and Hf 2-2
| display-authors=1 | last1=McNabb | first1=I. A.
| last2=Fang | first2=X. | last3=Liu | first3=X. -W.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=461 | issue=3 | pages=2818–2846 | date=September 2016
| doi=10.1093/mnras/stw1405 | doi-access=free | arxiv=1606.02925
| bibcode=2016MNRAS.461.2818M }}</ref>

<ref name=Iben_et_al_1983>{{cite journal
| title=On the evolution of those nuclei of planetary nebulae that experience a final helium shell flash
| url=https://archive.org/details/sim_astrophysical-journal_1983-01-15_264_2/page/604
| last1=Iben | first1=I., Jr. | last2=Kaler | first2=J. B.
| last3=Truran | first3=J. W. | last4=Renzini | first4=A.
| display-authors=1 | journal=Astrophysical Journal
| volume=264 | pages=605–612 | date=January 1983
| doi=10.1086/160631 | bibcode=1983ApJ...264..605I }}</ref>

}}

== 進階讀物 ==
{{Div col|small=yes}}
*{{cite journal
| title=MUSE spectroscopy of the high abundance discrepancy planetary nebula NGC 6153
| last1=Gómez-Llanos | first1=V. | last2=García-Rojas | first2=J.
| last3=Morisset | first3=C. | last4=Monteiro | first4=H.
| last5=Jones | first5=D. | last6=Wesson | first6=R.
| last7=Boffin | first7=H. M. J. | last8=Corradi | first8=R. L. M.
| display-authors=1 | journal=Astronomy & Astrophysics
| volume=689 | at=id. A228 | date=September 2024
| doi=10.1051/0004-6361/202450822 | arxiv=2407.06385
| bibcode=2024A&A...689A.228G }}
*{{cite journal
| title=NGC 6153: Reality is Complicated
| display-authors=1 | last1=Richer | first1=Michael G.
| last2=Arrieta | first2=Anabel | last3=Arias | first3=Lorena
| last4=Castañeda-Carlos | first4=Lesly | last5=Torres-Peimbert
| first5=Silvia | last6=López | first6=José Alberto | last7=Galindo | first7=Adolfo
| journal=The Astronomical Journal
| volume=164 | issue=6 | at=id. 243 | date=December 2022
| doi=10.3847/1538-3881/ac9732 | doi-access=free | arxiv=2210.05085
| bibcode=2022AJ....164..243R }}
*{{cite journal
| title=NGC 6153: a super-metal-rich planetary nebula?
| url=https://archive.org/details/sim_monthly-notices-of-the-royal-astronomical-society_2000-03-01_312_3/page/584
| last1=Liu | first1=X. -W. | last2=Storey | first2=P. J.
| last3=Barlow | first3=M. J. | last4=Danziger | first4=I. J.
| last5=Cohen | first5=M. | last6=Bryce | first6=M.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=312 | issue=3 | pages=585–628 | date=March 2000
| doi=10.1046/j.1365-8711.2000.03167.x
| doi-access=free | bibcode=2000MNRAS.312..585L | display-authors=1 }}
*{{cite journal
| title=Chemical Abundances of Planetary Nebulae: A UV to Far-IR Case Study of NGC 6153
| last=Liu | first=X. -W.
| journal=Astrophysics and Space Science
| volume=255 | issue=1/2 | pages=499–505 | year=1998
| doi=10.1023/A:1001515704001 | bibcode=1998Ap&SS.255..499L }}
{{Div col end}}

== 外部連結 ==
* {{commons category-inline}}
* {{cite simbad
| title=NGC 6153
| accessdate=2013-09-06 }}

{{Ngc65}}
{{天蠍座}}
[[Category:行星狀星雲]]
[[Category:天蠍座]]
[[Category:NGC天體|6153]]

NGC 6153 - 版本历史

imported>InternetArchiveBot：​Add 3 books for verifiability (20251017sim)) #IABot (v2.0.9.5) (GreenC bot

imported>InternetArchiveBot：Add 3 books for verifiability (20251017sim)) #IABot (v2.0.9.5) (GreenC bot