WOH G64: Perbedaan antara revisi
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Baris 39:
| dist_ly=160,000
| dist_pc=50,000<ref name=levesque/>
| absmag_v =
}}
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Baris 45:
| radius={{val|1,540|77|fmt=commas}}<ref name=levesque/> - 1,730<ref name=ohnaka/>
| luminosity={{val|282,000|40,000|30,000|fmt=commas}}<ref name=levesque/><ref name=ohnaka>{{Cite journal | last1 = Ohnaka | first1 = K. | last2 = Driebe | first2 = T. | last3 = Hofmann | first3 = K. H. | last4 = Weigelt | first4 = G. | last5 = Wittkowski | first5 = M. | title = Resolving the dusty torus and the mystery surrounding LMC red supergiant WOH G64 | doi = 10.1017/S1743921308028858 | journal = Proceedings of the International Astronomical Union | volume = 4 | pages = 454–458 | year = 2009 | pmid = | pmc = | bibcode = 2009IAUS..256..454O | doi-access = free }}</ref> {{nowrap|(340,000 – 454,000)<ref name=steven>{{cite journal|arxiv=1610.05761|bibcode=2017MNRAS.465..403G|doi=10.1093/mnras/stw2708|author1=Steven R. Goldman|author2=Jacco Th. van Loon|title=The wind speeds, dust content, and mass-loss rates of evolved AGB and RSG stars at varying metallicity|year=2016|journal=[[Monthly Notices of the Royal Astronomical Society]]|volume=465|issue=1|pp=403-433}}</ref>}}
| temperature=3,200<ref name=ohnaka/> - {{val|3,400|25|fmt=commas}},<ref name=levesque/>
| metal=
| rotation=
Baris 58:
}}
{{Starbox end}}
[[Berkas:WOH G64 Particular.jpg|thumb|left|upright=1.2|Kesan seniman tentang torus yang berdebu di sekitar WOH G64 ( [[Observatorium Selatan Eropa]] )]]▼
'''WOH G64''' adalah bintang merah raksasa di [[Awan Magellan Besar]]. Dengan jari-jari 2000 kali lebih besar dari [[matahari]], bintang ini adalah [[daftar bintang terbesar|bintang terbesar kedua]].▼
▲'''WOH G64''' adalah bintang merah raksasa di [[Awan Magellan Besar]]. Dengan
Ukuran WOH G64 diperkirakan sekitar 2.143.000.000 km, atau 1540 radii.<ref>^ E. M. Levesque. "WOH G64: The Largest Star Known?". Astronomical Journal. http://adsabs.harvard.edu/abs/2009AJ....137.4744L. Retrieved 2010-07 16.</ref>▼
▲Ukuran WOH G64 diperkirakan sekitar 2.143.000.000
== Penemuan ==
WOH G64 ditemukan pada 1970-an oleh [[Bengt Westerlund]] , Olander dan Hedin. Seperti NML Cygni , "WOH" dalam nama bintang berasal dari nama tiga penemunya, tetapi dalam hal ini mengacu pada seluruh katalog bintang raksasa dan [[supergiant]] di LMC.
Pada 2007, pengamat menggunakan [[Very Large Telescope]] (VLT) menunjukkan bahwa WOH G64 dikelilingi oleh awan berbentuk [[torus]].
== Jarak ==
▲[[Berkas:WOH G64 Particular.jpg|thumb|left|upright=1.2|Kesan seniman tentang torus yang berdebu di sekitar WOH G64 ( [[Observatorium Selatan Eropa]] )]]
Jarak WOH G64 diasumsikan sekitar 50.000 [[parsec]] (160.000 [[Tahun cahaya|ly]] ) jauhnya dari [[Bumi]], karena tampaknya berada di LMC.
== Variabilitas ==
Baris 83 ⟶ 84:
== Lihat pula ==
*[[UY Scuti]]
== Referensi ==
<ref name=2mass>{{cite journal |bibcode=2003yCat.2246....0C |title=VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) |journal=CDS/ADC Collection of Electronic Catalogues |pages=II/246 |volume=2246 |last1=Cutri |first1=Roc M. |last2=Skrutskie |first2=Michael F. |last3=Van Dyk |first3=Schuyler D. |last4=Beichman |first4=Charles A. |last5=Carpenter |first5=John M. |last6=Chester |first6=Thomas |last7=Cambresy |first7=Laurent |last8=Evans |first8=Tracey E. |last9=Fowler |first9=John W. |last10=Gizis |first10=John E. |last11=Howard |first11=Elizabeth V. |last12=Huchra |first12=John P. |last13=Jarrett |first13=Thomas H. |last14=Kopan |first14=Eugene L. |last15=Kirkpatrick |first15=J. Davy |last16=Light |first16=Robert M. |last17=Marsh |first17=Kenneth A. |last18=McCallon |first18=Howard L. |last19=Schneider |first19=Stephen E. |last20=Stiening |first20=Rae |last21=Sykes |first21=Matthew J. |last22=Weinberg |first22=Martin D. |last23=Wheaton |first23=William A. |last24=Wheelock |first24=Sherry L. |last25=Zacarias |first25=N. |year=2003 |url=http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=II/246 }}</ref>
<ref name=vanloon>{{cite journal|bibcode=2005A&A...438..273V|arxiv=astro-ph/0504379|title=An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars|journal=Astronomy and Astrophysics|volume=438|pages=273–289|last1=Van Loon|first1=J. Th.|last2=Cioni|first2=M.-R. L.|last3=Zijlstra|first3=A. A.|last4=Loup|first4=C.|year=2005|issue=1|doi=10.1051/0004-6361:20042555|s2cid=16724272}}</ref>
<ref name=ogle>{{cite journal|bibcode=2009AcA....59..239S|title=The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. IV. Long-Period Variables in the Large Magellanic Cloud|journal=Acta Astronomica|volume=59|issue=3|pages=239|last1=Soszyñski|first1=I.|last2=Udalski|first2=A.|last3=Szymañski|first3=M. K.|last4=Kubiak|first4=M.|last5=Pietrzyñski|first5=G.|last6=Wyrzykowski|first6=Ł.|last7=Szewczyk|first7=O.|last8=Ulaczyk|first8=K.|last9=Poleski|first9=R.|year=2009|arxiv=0910.1354}}</ref>
}}
== Bibliografi ==
* {{cite journal |last=Westerlund |first=B. E. |authorlink= |coauthors=Olander, N.; Hedin, B. |year=1981 |month= |title=Supergiant and giant M type stars in the Large Magellanic Cloud |journal=Astronomy & Astrophysics Suppl. Ser. |volume=43 |issue= |pages=267–295 |id= |url= |accessdate= |quote= }}
* {{cite journal |last=Ohnaka |first=K. |authorlink= |coauthors=''et al.'' |year=2008 |month= |title=Spatially resolved dusty torus toward the red supergiant WOH G64 in the Large Magellanic Cloud |journal=Astronomy & Astrophysics |volume=484 |issue= |pages=371–379 |doi=10.1051/0004-6361:200809469 |url= |accessdate= |quote= }}
▲{{reflist}}
[[Kategori:Bintang]]
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