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The Veil Nebula is a cloud of heated and ionized gas and dust in the constellation Cygnus. [ 4 ] It constitutes the visible portions of the Cygnus Loop , [ 5 ] a supernova remnant , many portions of which have acquired their own individual names and catalogue identifiers.
The Cygnus Loop (radio source W78, or Sharpless 103) is a large supernova remnant (SNR) in the constellation Cygnus, an emission nebula measuring nearly 3° across. [1] Some arcs of the loop, known collectively as the Veil Nebula or Cirrus Nebula, emit in the visible electromagnetic range. [1] Radio, infrared, and X-ray images reveal the ...
NGC 6992 (Eastern Veil Nebula – center) and NGC 6960 (Western Veil Nebula – upper right) photographed from a dark site. To the south of Epsilon Cygni is the Veil Nebula (NGC 6960, 6979, 6992, and 6995), a 5,000-year-old supernova remnant covering approximately 3 degrees of the sky - [66] it is over 50 light-years long. [4]
52 Cygni with NGC 6960, part of the Veil Nebula. 52 Cygni is a giant star in the northern constellation of Cygnus with an apparent magnitude of 4.22. Based on its Hipparcos parallax, it is about 291 light-years (89 pc) away.
ε Cygni appears north of the Veil nebula towards the bottom left. Epsilon Cygni A is a single-lined spectroscopic binary. [18] Radial velocity observations suggest a possible companion with an orbital period of at least 15 years. [16] It presents as a giant star with a stellar classification of K0 III. [19]
An emission nebula is a nebula formed of ionized gases that emit light of various wavelengths. ... (NGC 7000) and Veil Nebula NGC 6960/6992 in Cygnus, ...
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NGC 6871 is a small, young open cluster in the constellation of Cygnus.The cluster has fewer than 50 members, most of which are blue and white stars. It is located 5135 light-years from Earth.