{"id":8328,"date":"2019-08-05T12:42:49","date_gmt":"2019-08-05T11:42:49","guid":{"rendered":"http:\/\/outters.fr\/?p=8328"},"modified":"2025-07-15T17:04:07","modified_gmt":"2025-07-15T16:04:07","slug":"snr_g065-2-hoo-rgb","status":"publish","type":"post","link":"https:\/\/www.outters.fr\/?p=8328","title":{"rendered":"SNR G065.2+05.7 HOO-rgb"},"content":{"rendered":"

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SNR G065.2+05.7 HOO-rgb<\/span><\/p><\/h2><\/span>

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Donn\u00e9es techniques de prise de vue<\/h2><\/div>
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Object : SNR G065.2+05.7
\nCommon name :
\nDate : du 22 juin au\u00a0 3 aout 2019
\nOptics : Newton OO400 F3,8
\nMount : Paramount ME Num\u00e9ro 1
\nLocation : Orange observatory
\nSeeing FWHM :2.43 \u00e0 5.7
\nCcd : Moravian G4
\nfilter wheel : Moravian
\nfilters : Astrodon LRVB
\nFocuser :Atlas
\nGuiding : Atik 314L+
\nTemp. out : T\u00b0 de 10.9 \u00b0
\nTemp ccd : -25\u00b0
\nResolution ………….. 1.221 arcsec\/px
\nRotation ……………. -6.122 deg
\nObservation date …….. 2019-06-28 01:50:39
\nGeodetic coordinates …. 6 19 04 W 46 01 49 N
\nFocal distance ………. 1519.96 mm
\nPixel size ………….. 9.00 um
\nField of view ……….. 1d 23′ 22.6″ x 1d 23′ 22.6″
\nImage center ………… RA: 19 28 10.851 Dec: +31 24 58.28
\nTotal exposure 19.75 h
\ntout en binning 1×1
\nHa 44 x 10mn
\nOIII 49 x 10 mn
\n18R 15V 18B x 5mn<\/p>\n<\/div><\/div><\/div>

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Image HOO-rgb<\/h2><\/a><\/div><\/div><\/div>
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Image HO invers\u00e9e<\/h2><\/a><\/div><\/div><\/div>
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Commentaires sur l’objet photographi\u00e9<\/span><\/p><\/h1><\/span>

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Cette image du r\u00e9manent de supernovae SNR G065.2+05.7 est une petite partie de cet ensemble immense.<\/p>\n

\"outters-nicolas\"<\/p>\n<\/div>

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Donn\u00e9es techniques
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Source https:\/\/www.cxielo.ch\/gallery\/f\/g65<\/p>\n

Little Veil Nebula (SNR G065.2+05.7)<\/h2>\n


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\nG65.2+5.7 is a SNR in the constellation of Cygnus, similar to the well known Cygnus Loop. It was discovered 1977 by T.R. Gull and covers an area of about 3.5\u00b0 x 4.0\u00b0. Because of G65.3+5.7 large distance (about 2500 lightyears) and higher age (about 30’000 years), the filaments are very faint. Parts of the filametary structures have been catalogued as SH2-91, SH2-94 and SH2-96.<\/p>\n

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