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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]
Western part of Veil Nebula 'Witch Broom' Diffuse nebula: Cygnus: 20 h 45 m 38.0 s +30° 42′ 30″ 6981: Messier 72 Globular cluster: Aquarius: 20 h 53 m 27.9 s: −12° 32′ 13″ 10.0 6992: Eastern part of the Veil Nebula 'Banana Nebula' Diffuse nebula: Cygnus: 20 h 57 m +31° 30′ 6994: Messier 73 Asterism [7] Aquarius: 20 h 59 m: −12 ...
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.
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, ...
The lace veil — technically called a mantilla — has been worn in the presence of a Pope by many former first ladies, including Jackie Kennedy, Pat Nixon, Betty Ford, Rosalynn Carter, Nancy ...
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]