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"गांगेय केंद्र": अवतरणों में अंतर

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[[Image:Galactic Cntr full cropped.jpg|thumb|350px|right|Tदो मास इंफ्रारेड टेलीस्कोपों में से एक में दिखा गांगेय केंद्र, छवि के ऊपरी बाएं आलोकित भाग में स्थित है । ]]
'''गांगेय केंद्र''' (Galactic Center), हमारी आकाशगंगा का घूर्णी केंद्र है | यह हमारी [[पृथ्वी]] से 8.33±0.35 kpc (~27,000±1,000 प्रकाश वर्ष) की दूरी पर स्थित है । <ref name="distance1">{{cite journal|last = Reid|first = Mark J.|title=The distance to the center of the Galaxy|journal=Annual review of astronomy and astrophysics|year=1993|volume=31|issue = 1| pages=345–372|bibcode=1993ARA&A..31..345R|accessdate=2007-05-10|doi= 10.1146/annurev.aa.31.090193.002021}}</ref><ref name="distance2">{{cite journal|author=Eisenhauer, F.; Schödel, R.; Genzel, R.; Ott, T.; Tecza, M.; Abuter, R.; Eckart, A.; Alexander, T.|title=A Geometric Determination of the Distance to the Galactic Center| journal=The Astrophysical Journal|year=2003|volume=597|issue=2|pages=L121–L124|bibcode=2003ApJ...597L.121E | arxiv=astro-ph/0306220|doi=10.1086/380188}}</ref><ref name="distance3">{{cite journal|author=Horrobin, M.; Eisenhauer, F.; Tecza, M.; Thatte, N.; Genzel, R.; Abuter, R.; Iserlohe, C.; Schreiber, J.; Schegerer, A.; Lutz, D.; Ott, T.; Schödel, R.|title=First results from SPIFFI. I: The Galactic Center|journal=Astronomische Nachrichten|year=2004|volume=325|issue=2|pages=120–123|url= http://www.mpe.mpg.de/SPIFFI/preprints/first_result_an1.pdf|format=PDF|accessdate=2007-05-10|doi=10.1002/asna.200310181|bibcode=2004AN....325...88H}}</ref><ref name=majaess2009>Majaess D. J., Turner D. G., Lane D. J. (2009). [http://adsabs.harvard.edu/abs/2009arXiv0903.4206M ''Characteristics of the Galaxy according to Cepheids''], MNRAS</ref><ref name=gillessenetal2009>{{cite journal|last=Gillessen| first = S.|coauthors=Eisenhauer; Trippe; Alexander; Genzel; Martins; Ott|title=Monitoring Stellar Orbits Around the Massive Black Hole in the Galactic Center|journal=The Astrophysical Journal|volume=692|issue=2|pages=1075–1109|year=2009|doi=10.1088/0004-637X/692/2/1075|accessdate=2010-10-28|bibcode=2009ApJ...692.1075G|arxiv=0810.4674}}</ref> यह [[धनु तारामंडल|धनु]], [[सर्पधारी तारामंडल|सर्पधारी ]], और [[वॄश्चिक तारामंडल|वृश्चिक]] [[तारामंडल]] की दिशा में स्थित है जहां हमारी आकाशगंगा उज्जवल प्रतीत होती है | Thereइस isबात strongके evidenceपुख्ता thatप्रमाण supportsहै theजो existenceहमारी ofआकाशगंगा के गांगेय केंद्र में aएक [[supermassiveविशालकाय blackब्लैक holeहोल]] atके theवजुद Galacticका Centerसमर्थन ofकरता theहै [[Milky। Way]].▼
[[File:Infrared-visible light comparison of VISTA’s gigapixel view of the centre of the Milky Way.ogv|thumb|350px|This pan video gives a closer look at a huge image of the central parts of the Milky Way made by combining thousands of images from ESO’s [[VISTA (telescope)|VISTA telescope]] on Paranal in Chile and compares it with the view in visible light. Because VISTA has a camera sensitive to infrared light it can see through much of the dust blocking the view in visible light, although many more opaque dust filaments still show up well in this picture.]]
 
▲'''गांगेय केंद्र''' (Galactic Center), हमारी आकाशगंगा का घूर्णी केंद्र है | यह हमारी [[पृथ्वी]] से 8.33±0.35 kpc (~27,000±1,000 प्रकाश वर्ष) की दूरी पर स्थित है । <ref name="distance1">{{cite journal|last = Reid|first = Mark J.|title=The distance to the center of the Galaxy|journal=Annual review of astronomy and astrophysics|year=1993|volume=31|issue = 1| pages=345–372|bibcode=1993ARA&A..31..345R|accessdate=2007-05-10|doi= 10.1146/annurev.aa.31.090193.002021}}</ref><ref name="distance2">{{cite journal|author=Eisenhauer, F.; Schödel, R.; Genzel, R.; Ott, T.; Tecza, M.; Abuter, R.; Eckart, A.; Alexander, T.|title=A Geometric Determination of the Distance to the Galactic Center| journal=The Astrophysical Journal|year=2003|volume=597|issue=2|pages=L121–L124|bibcode=2003ApJ...597L.121E | arxiv=astro-ph/0306220|doi=10.1086/380188}}</ref><ref name="distance3">{{cite journal|author=Horrobin, M.; Eisenhauer, F.; Tecza, M.; Thatte, N.; Genzel, R.; Abuter, R.; Iserlohe, C.; Schreiber, J.; Schegerer, A.; Lutz, D.; Ott, T.; Schödel, R.|title=First results from SPIFFI. I: The Galactic Center|journal=Astronomische Nachrichten|year=2004|volume=325|issue=2|pages=120–123|url= http://www.mpe.mpg.de/SPIFFI/preprints/first_result_an1.pdf|format=PDF|accessdate=2007-05-10|doi=10.1002/asna.200310181|bibcode=2004AN....325...88H}}</ref><ref name=majaess2009>Majaess D. J., Turner D. G., Lane D. J. (2009). [http://adsabs.harvard.edu/abs/2009arXiv0903.4206M ''Characteristics of the Galaxy according to Cepheids''], MNRAS</ref><ref name=gillessenetal2009>{{cite journal|last=Gillessen| first = S.|coauthors=Eisenhauer; Trippe; Alexander; Genzel; Martins; Ott|title=Monitoring Stellar Orbits Around the Massive Black Hole in the Galactic Center|journal=The Astrophysical Journal|volume=692|issue=2|pages=1075–1109|year=2009|doi=10.1088/0004-637X/692/2/1075|accessdate=2010-10-28|bibcode=2009ApJ...692.1075G|arxiv=0810.4674}}</ref> [[धनु]], [[सर्पधारी तारामंडल|सर्पधारी ]], और [[वृश्चिक]] [[तारामंडल]] की दिशा में स्थित है जहां हमारी आकाशगंगा उज्जवल प्रतीत होती है | There is strong evidence that supports the existence of a [[supermassive black hole]] at the Galactic Center of the [[Milky Way]].
 
==सन्दर्भ==
"https://hi.wikipedia.org/wiki/गांगेय_केंद्र" से प्राप्त