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Dear group,
Third time lucky in my attempts to image Sh2-96 and which represents the northern section of the shell of the supernova remnant G65.2+05.7 (the western wall of the shell is represented by Sh2-94 and the southern section of the shell by Sh2-91). The identification of G65.2+05.7 occurred in 1977 during an emission line survey of the galactic plane and where the various pieces were finally put together, thus identifying this large area of emission nebulosity as a supernova remnant. For last night's result under good seeing and transparency, please see http://www.perseus.gr/Astro-DSO-Nebulae-Sh2-96.htm . Anthony. |
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On 8/28/11 7:20 AM, Anthony Ayiomamitis wrote:
Dear group, Third time lucky in my attempts to image Sh2-96 and which represents the northern section of the shell of the supernova remnant G65.2+05.7 (the western wall of the shell is represented by Sh2-94 and the southern section of the shell by Sh2-91). The identification of G65.2+05.7 occurred in 1977 during an emission line survey of the galactic plane and where the various pieces were finally put together, thus identifying this large area of emission nebulosity as a supernova remnant. For last night's result under good seeing and transparency, please see http://www.perseus.gr/Astro-DSO-Nebulae-Sh2-96.htm . Anthony. What an excellent week! Thanks Anthony. -Sam |
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