Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  12 Cyg  ·  12 phi Cyg  ·  17 Cyg  ·  2 Cyg  ·  3 Vul  ·  6 Cyg A)  ·  6 Cyg B  ·  6 bet01 Cyg  ·  6 bet02 Cyg  ·  8 Cyg  ·  9 Cyg  ·  Albireo  ·  NGC 6813  ·  NGC 6815  ·  PK061+02.1  ·  PK061+03.1  ·  PK064+05.1  ·  PK065+03.1  ·  Sh2-91  ·  Sh2-92  ·  Sh2-94  ·  Sh2-96  ·  The star 17 Cyg  ·  The star 2 Cyg  ·  The star 3 Vul  ·  The star 8 Cyg  ·  The star 9 Cyg  ·  The star Albireo (β1 Cyg  ·  The star β2 Cyg  ·  The star φ Cyg
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The invisible elephant in the room: Supernova Remnant SNR G065.2+05.7 in South Cygnus, Mau_Bard
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The invisible elephant in the room: Supernova Remnant SNR G065.2+05.7 in South Cygnus

Getting plate-solving status, please wait...
The invisible elephant in the room: Supernova Remnant SNR G065.2+05.7 in South Cygnus, Mau_Bard
Powered byPixInsight

The invisible elephant in the room: Supernova Remnant SNR G065.2+05.7 in South Cygnus

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This is a deprecated image. The new, better version is visible here!

I recorded the not-so-narrow-band data (L-eNhance filter has 10 nm Ha and 24nm OIII) during 4 night in July 2023, with my new Samyang 135 setup.
The left side of the picture is pointing North.

SNR G065.2+05.7
The picture covers the area of south Cygnus around Albireo, but its main character is the huge supernova remnant SNR G065.2+05.7, that covers an area of approximately 5 x 3 degrees (that is 6 x 10 moon diameters).
It is a real invisible elephant in the room: we observed this area many times without knowing that this giant is sitting there just in front of our eyes. Only it is too faint to be seen, and even in narrowband pictures its signal is extremely weak. The brighter portions of it have been numbered separately as Sh2- 91, 94 and 96.
It was detected as a single object by Gull et alii in 1977 during an optical survey. Estimates of its linear diameter is ~70 pc (230 ly) and its distance is 0.8+-0.2 kpc (~2600 ly). It age is about 20000 years.
The Ha and OIII signals are remarkably different, and the Ha is mixing up with the emission background, therefore it is not easy to understand the shape of the object. The second article quoted below states that SNR G065.2+05.7 is an example of a barrel–shaped supernova remnant. Initially I thought that the Sh2-96 area was a "Champagne flow", but I have found no statement about that.
Interesting is the 2002 article by the University of Crete, Physics Department and this other.
A nice page has been dedicated to it by Stephane Zoll.
I came to know about it and was inspired by the beautiful image of @Walter Leonhard Schramböck.

Sh2-92
Sh 2-92 is ionized by the Wolf-Rayet star WR 127, a binary star with an O9V companion.

Sh2-91, Sh2-94 and Sh2-96
As already mentioned these are all filaments of the supernova remnant SNR G065.2+05.7.

NGC6813
NGC6813 and several other planetary nebulae are visible in the picture.

NGC6815
NCG6815 is just an association of stars in Vulpecula, discovered by John Herschel in 1828.

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