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The Algol system as it appeared on 12 August 2009. This is not an artistic representation, but rather is a true two-dimensional image with 1/2 milli-arcsecond resolution in the near-infrared H-band, reconstructed from data of the CHARA interferometer. The elongated appearance of Algol B and the round
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791:{{Information |Description ={{en|1=The Algol system as it appeared on 12 August 2009. This is not an artistic representation, but rather is a true two-dimensional image with 1/2 milli-arcsecond resolution in the near-infrared H-band, reconstructed f...
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The
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This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
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If the file has been modified from its original state, some details may not fully reflect the modified file.
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The following pages on the
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https://ticket.wikimedia.org/otrs/index.pl?Action=AgentTicketZoom&TicketNumber=2012100410002832
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Dr Fabien Baron, Dept. of
Astronomy, University of Michigan, Ann Arbor, MI 48109-1090
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appearance of Algol A are real. The form of Algol C, however, is a artifact.
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If you have questions about the archived correspondence, please use the
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Algol triple star system imaged with the CHARA interferometer.jpg
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Algol_triple_star_system_imaged_with_the_CHARA_interferometer.jpg
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http://www.oculum.de/newsletter/astro/100/60/2/2-01_algol.jpg
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and may be used by anyone for any purpose. If you wish to
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Commons is a freely licensed media file repository.
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854:Korisnik:Palapa/Zvjezdani sistem
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81:. Information from its
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1034:Кратна зоря
1014:ระบบดาวฤกษ์
979:Star system
816:Star system
521:11 May 2012
414:copyrighted
320:share alike
314:attribution
137:11 May 2012
114:Description
797:File usage
778:350 × 159
754:Dimensions
555:image/jpeg
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161:Permission
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751:Thumbnail
748:Date/Time
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106:Summary
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949:Алголь
780:(6 KB)
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17:File
1044:大陵五
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