enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. List of supernova remnants - Wikipedia

    en.wikipedia.org/wiki/List_of_supernova_remnants

    This is a list of observed supernova remnants (SNRs) in the Milky Way, ... Spaghetti Nebula 05 h 39 m +27° 50′ ~40,000 years ago: 6.5: 3,000? neutron star PSR ...

  3. Supernova remnant - Wikipedia

    en.wikipedia.org/wiki/Supernova_remnant

    SN 1054 remnant (Crab Nebula).. A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova.The supernova remnant is bounded by an expanding shock wave, and consists of ejected material expanding from the explosion, and the interstellar material it sweeps up and shocks along the way.

  4. Nova remnant - Wikipedia

    en.wikipedia.org/wiki/Nova_remnant

    This theoretically means these nebula shapes might be affected by their central progenitor stars and the amount of matter ejected by novae. [1] The shapes of these nova nebulae are of much interest to modern astrophysicists. [1] [4] Nova remnants when compared to supernova remnants or planetary nebulae generate

  5. Category:Supernova remnants - Wikipedia

    en.wikipedia.org/wiki/Category:Supernova_remnants

    العربية; Беларуская; Български; Bosanski; Ελληνικά; Español; Esperanto; فارسی; Français; 한국어; हिन्दी; Italiano

  6. SN 1181 - Wikipedia

    en.wikipedia.org/wiki/SN_1181

    Before 2013, the only plausible conventional supernova remnant in the old historical area for the supernova was the supernova remnant 3C 58. This remnant has a radio and X-ray pulsar that rotates about 15 times per second. So historically, SN 1181 had been associated with 3C 58 and its pulsar, although many researchers noted that this ...

  7. IRAS 00500+6713 - Wikipedia

    en.wikipedia.org/wiki/IRAS_00500+6713

    Analysis of X-ray spectra allowed for the first time to determine the chemical composition of the nebula. It was proposed that the nebula is a remnant of a rare type of supernova (SN Iax), and that the SN happened some 1000 years ago. [3] It has been linked to the historic supernova SN 1181. [4]

  8. Cassiopeia A - Wikipedia

    en.wikipedia.org/wiki/Cassiopeia_A

    Cassiopeia A (Cas A) (listen ⓘ) is a supernova remnant (SNR) in the constellation Cassiopeia and the brightest extrasolar radio source in the sky at frequencies above 1 GHz. The supernova occurred approximately 11,000 light-years (3.4 kpc ) away within the Milky Way ; [ 2 ] [ 3 ] given the width of the Orion Arm , it lies in the next-nearest ...

  9. 3C 58 - Wikipedia

    en.wikipedia.org/wiki/3C_58

    A second conclusive argument is that the real remnant of SN 1181 was discovered by American amateur astronomer Dana Patchik, designated Pa 30. Pa 30 is known from multiple independent measures to be a supernova remnant with an age close to 800 years, and it is inside the modern sky position for the 1181 supernova.