File:Diffraktion Delta Lyrae.png

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Deutsch: Beugung durch ein Teleskop: Bei δ2 Lyrae sind mehrere Beugungsscheibchen deutlich erkennbar, während bei den umliegenden Sternen nur das jeweils innerste Beugungsscheibchen klar sichtbar ist.
Source δ Lyrae in DSS colored - Digitized Sky Survey - STScI/NASA, Colored & Healpixed by CDS, 18 53 31.603 +36 51 24.12, FoV: 37.19'
Author Kersti (talk) 06:53, 12 August 2023 (UTC) using The ALADIN interactive sky atlas, aladin.unistra.fr, DSS colored - Digitized Sky Survey - STScI/NASA

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Date/TimeThumbnailDimensionsUserComment
current06:53, 12 August 2023Thumbnail for version as of 06:53, 12 August 20231,923 × 1,730 (4.38 MB)Kersti Nebelsiek (talk | contribs){{Information |Description={{de|Beugung durch ein Teleskop: Bei δ2 Lyrae sind mehrere Beugungsscheibchen deutlich erkennbar, während bei den umliegenden Sternen nur das jeweils innerste Beugungsscheibchen klar sichtbar ist.}} |Source=[https://aladin.cds.unistra.fr/AladinLite/?target=18%2054%2030.283%2B36%2053%2055.01&fov=0.62&survey=P%2FDSS2%2Fcolor δ Lyrae in DSS colored - Digitized Sky Survey - STScI/NASA, Colored & Healpixed by CDS, 18 53 31.603 +36 51 24.12, FoV: 37.19'] |Date= |Author=~...

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