小麦哲伦星系:修订间差异
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{{Infobox galaxy |
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{{Galaxy |
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|name = 小麥哲倫星系(SMC) |
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|image = [[File:Small Magellanic Cloud (Digitized Sky Survey 2).jpg|300px]] |
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|caption = 小麥哲倫星系<br/>(Source: [[數位化巡天項目]] 2) |
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|[[可見光和紅外巡天望遠鏡|VISTA]]拍攝的小麥哲倫星系,右方是[[球狀星團]][[NGC 104]]<br /></small> |
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|epoch = [[曆元#儒略年和J2000|J2000]] |
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|type = SB(s)m pec<ref name="ned">{{cite web |
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|title=NASA/IPAC 河外資料庫 |
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|work=小麥哲倫星系的結果 |
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| work=Results for Small Magellanic Cloud |
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|url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=Small+Magellanic+Cloud&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 |
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| url=http://nedwww.ipac.caltech.edu/ |
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| access-date=2006-12-01 }}</ref> |
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| archive-date=2011-05-14 |
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| archive-url=https://web.archive.org/web/20110514100451/http://nedwww.ipac.caltech.edu/ |
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| dead-url=no |
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}}</ref> |
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| ra = {{RA|00|52|44.8}}<ref name="ned" /> |
| ra = {{RA|00|52|44.8}}<ref name="ned" /> |
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| dec = {{DEC|-72|49|43}}<ref name="ned" /> |
| dec = {{DEC|-72|49|43}}<ref name="ned" /> |
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| dist_ly = [[1 E20 m|203.7 ± 1.5]] [[光年|kly]] (62.44 ± 0.47 [[秒差距|kpc]])<ref name=Graczyk2020>{{cite journal | doi=10.3847/1538-4357/abbb2b | title=A Distance Determination to the Small Magellanic Cloud with an Accuracy of Better than Two Percent Based on Late-type Eclipsing Binary Stars | year=2020 | last1=Graczyk | first1=Dariusz | last2=Pietrzyński | first2=Grzegorz | last3=Thompson | first3=Ian B. | last4=Gieren | first4=Wolfgang | last5=Zgirski | first5=Bartłomiej | last6=Villanova | first6=Sandro | last7=Górski | first7=Marek | last8=Wielgórski | first8=Piotr | last9=Karczmarek | first9=Paulina | last10=Narloch | first10=Weronika | last11=Pilecki | first11=Bogumił | last12=Taormina | first12=Monica | last13=Smolec | first13=Radosław | last14=Suchomska | first14=Ksenia | last15=Gallenne | first15=Alexandre | last16=Nardetto | first16=Nicolas | last17=Storm | first17=Jesper | last18=Kudritzki | first18=Rolf-Peter | last19=Kałuszyński | first19=Mikołaj | last20=Pych | first20=Wojciech | journal=The Astrophysical Journal | volume=904 | issue=1 | page=13 | arxiv=2010.08754 | bibcode=2020ApJ...904...13G | s2cid=224706414 | doi-access=free }}</ref> |
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| dist_ly = [[1 E20 m|197 ± 9]] [[light-year|kly]] (61 ± 3 [[parsec|kpc]])<ref name="Gierenetal2005">{{cite journal |
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| author=Hilditch, R. W.; Howarth, I. D.; Harries, T. J. |
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|appmag_v = 2.7<ref name="ned" /> |
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| year=2005 |
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⚫ | |||
| title=Forty eclipsing binaries in the Small Magellanic Cloud: fundamental parameters and Cloud distance |
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|size = {{convert|5.78|kpc|ly|sigfig=3|abbr=off}}<ref name="ned" /><br />(直徑:25.0 mag/arcsec<sup>2</sup> B-頻道等電位)<ref name=RC3>{{cite book | url=https://ui.adsabs.harvard.edu/abs/1991rc3..book.....D | bibcode=1991rc3..book.....D | year=1991 | title=Third Reference Catalogue of Bright Galaxies | last1=De Vaucouleurs | first1=Gerard | last2=De Vaucouleurs | first2=Antoinette | last3=Corwin | first3=Herold G. | last4=Buta | first4=Ronald J. | last5=Paturel | first5=Georges | last6=Fouque | first6=Pascal }}</ref> |
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| journal=Monthly Notices of the Royal Astronomical Society |
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|stars=30億<ref>{{cite book | author = Jonathan Powell | date = 17 September 2018 | title = Rare Astronomical Sights and Sounds | publisher = Springer | pages = | isbn = 978-3-319-97701-0 | url = https://books.google.com/books?id=Df5uDwAAQBAJ}}</ref> |
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| volume=357 |
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| issue=1 |
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|notes = Companion dwarf to the [[銀河系]]的<br/>侏儒夥伴 |
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| pages=304-324 |
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| url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005MNRAS.357..304H }}</ref> |
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| z = 158 ± 4 [[kilometer|km]]/[[second|s]]<ref name="ned" /> |
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| notes = [[銀河系]]的矮衛星星系 |
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}} |
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{{NGCInfoBox|NGCID=NGC 292|發現者=麥哲倫|發現日期=1521年-月-日|其他編號=ESO 29-21,A 0051-73,IRAS00510-7306|曆元=J2000.0|赤經=52分38秒|赤緯=-72°48'0""|星座=杜鹃座|星體=不規則星系|星等=2.2|表面亮度=14.1|藍等=2.8}} |
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'''小麥哲倫星系'''(SMC)是一個環繞著[[銀河系]]的[[矮星系]]<ref name="#1">{{Cite web |url=http://antwrp.gsfc.nasa.gov/apod/ap050617.html |title=存档副本 |accessdate=2007-02-10 |archive-date=2010-08-08 |archive-url=https://web.archive.org/web/20100808205833/http://antwrp.gsfc.nasa.gov/apod/ap050617.html |dead-url=no }}</ref>,擁有數億顆的恆星 <ref name="#1"/>。 |
'''小麥哲倫星系'''(SMC)是一個環繞著[[銀河系]]的[[矮星系]]<ref name="#1">{{Cite web |url=http://antwrp.gsfc.nasa.gov/apod/ap050617.html |title=存档副本 |accessdate=2007-02-10 |archive-date=2010-08-08 |archive-url=https://web.archive.org/web/20100808205833/http://antwrp.gsfc.nasa.gov/apod/ap050617.html |dead-url=no }}</ref>,擁有數億顆的恆星 <ref name="#1"/>。 |
2024年1月17日 (三) 17:23的版本
小麥哲倫星系(SMC) | |
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小麥哲倫星系 (Source: 數位化巡天項目 2) | |
观测资料(J2000 曆元) | |
星座 | 杜鵑座和水蛇座 |
赤经 | 00h 52m 44.8s[1] |
赤纬 | -72° 49′ 43″[1] |
紅移 | 0.000527[1] |
距离 | 203.7 ± 1.5 kly (62.44 ± 0.47 kpc)[2] |
视星等 (V) | 2.7[1] |
特征 | |
类型 | SB(s)m pec[1] |
恒星数量 | 30億[4] |
大小 | 5.78千秒差距(18,900光年)[1] (直徑:25.0 mag/arcsec2 B-頻道等電位)[3] |
角直徑 (V) | 5° 20′ × 3° 5′[1] |
其他 | Companion dwarf to the 銀河系的 侏儒夥伴 |
其他名称 | |
SMC,[1] NGC 292[1], PGC 3085[1]、Nubecula Minor[1] | |
小麥哲倫星系(SMC)是一個環繞著銀河系的矮星系[5],擁有數億顆的恆星 [5]。
推測小麥哲倫星系原本是棒旋星系,因為受到銀河系的擾動才成為不規則星系 [6],但在核心仍殘留著棒狀的結構。
在20萬光年距離上的小麥哲倫星系是最靠近銀河系的鄰居之一,也是裸眼能看見的最遙遠天體之一。
他位於杜鵑座,在夜空中看似模糊的光斑,大小約為3゜,由於平均的赤緯是 -73゜,所以只能在南半球和北半球的低緯度地區看見。他看似銀河系被分割的一個片段,由於表面光度很低,要在黑暗的環境下才能看得清楚。
他與在東方20゜的大麥哲倫星系成為一對,都是本星系群的成員。
迷你麥哲倫雲
早在1986年,天體物理學家D.S.Mathewson、V.L.Ford和N.Visvanathan提出,事實上,小麥哲倫星系可能被一分為二,在它的主要部份後面有一小部分星系(從地球的角度來看),並相距約30,000光年。他們認為,這是由於過去與大麥哲倫星系的互動導致小麥哲倫星系分裂,並且這兩個部分仍在分離。他們將這個較小的遺跡命名為迷你麥哲倫星雲[7][8]。
2023年,據報導,小麥哲倫星系實際上是兩個獨立的結構,具有不同的恆星和氣體化學成分,相距約5,000秒差距[9]。
相關條目
參考資料
- ^ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 NASA/IPAC 河外資料庫. 小麥哲倫星系的結果. [2006-12-01].
- ^ Graczyk, Dariusz; Pietrzyński, Grzegorz; Thompson, Ian B.; Gieren, Wolfgang; Zgirski, Bartłomiej; Villanova, Sandro; Górski, Marek; Wielgórski, Piotr; Karczmarek, Paulina; Narloch, Weronika; Pilecki, Bogumił; Taormina, Monica; Smolec, Radosław; Suchomska, Ksenia; Gallenne, Alexandre; Nardetto, Nicolas; Storm, Jesper; Kudritzki, Rolf-Peter; Kałuszyński, Mikołaj; Pych, Wojciech. A Distance Determination to the Small Magellanic Cloud with an Accuracy of Better than Two Percent Based on Late-type Eclipsing Binary Stars. The Astrophysical Journal. 2020, 904 (1): 13. Bibcode:2020ApJ...904...13G. S2CID 224706414. arXiv:2010.08754 . doi:10.3847/1538-4357/abbb2b .
- ^ De Vaucouleurs, Gerard; De Vaucouleurs, Antoinette; Corwin, Herold G.; Buta, Ronald J.; Paturel, Georges; Fouque, Pascal. Third Reference Catalogue of Bright Galaxies. 1991. Bibcode:1991rc3..book.....D.
- ^ Jonathan Powell. Rare Astronomical Sights and Sounds. Springer. 17 September 2018. ISBN 978-3-319-97701-0.
- ^ 5.0 5.1 存档副本. [2007-02-10]. (原始内容存档于2010-08-08).
- ^ 存档副本. [2007-02-10]. (原始内容存档于2015-11-07).
- ^ Mathewson, D. S.; Ford, V. L.; Visvanathan, N. The structure of the Small Magellanic Cloud. The Astrophysical Journal. 1986, 301: 664. Bibcode:1986ApJ...301..664M. ISSN 0004-637X. doi:10.1086/163932.
- ^ Crowl, Hugh H.; et al. The Line-of-Sight Depth of Populous Clusters in the Small Magellanic Cloud. The Astronomical Journal. 2001, 122 (1): 220–231. Bibcode:2001AJ....122..220C. ISSN 0004-6256. S2CID 45263795. arXiv:astro-ph/0104227v1 . doi:10.1086/321128.
- ^ Murray, Claire E.; Hasselquist, Sten; Peek, Joshua E. G.; Christina Willecke Lindberg; Almeida, Andres; Choi, Yumi; Craig, Jessica E. M.; Denes, Helga; Dickey, John M.; Di Teodoro, Enrico M.; Federrath, Christoph; Gerrard, Isabella A.; Gibson, Steven J.; Leahy, Denis; Lee, Min-Young; Lynn, Callum; Yik Ki Ma; Marchal, Antoine; McClure-Griffiths, N. M.; Nidever, David; Nguyen, Hiep; Pingel, Nickolas M.; Tarantino, Elizabeth; Uscanga, Lucero; van Loon, Jacco Th. A Galactic Eclipse: The Small Magellanic Cloud is Forming Stars in Two, Superimposed Systems. 2023. arXiv:2312.07750 [astro-ph.GA].
外部連結
- NASA Extragalactic Database entry on the SMC (页面存档备份,存于互联网档案馆)
- SEDS entry on the SMC
- SMC at ESA/Hubble (页面存档备份,存于互联网档案馆)
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天文學目錄 | ||
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NGC天體表: | NGC 290 - NGC 291 - NGC 292 - NGC 293 - NGC 294 |
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