Magnetar

  • 21Pulsar — Pulsars are highly magnetized rotating neutron stars that emit a beam of electromagnetic radiation in the form of radio waves. Their observed periods range from 1.4 ms to 8.5 s. [ M.D. Young, R.N. Manchester and S. Johnston. A radio pulsar with… …

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  • 22SGR 1806-20 — Starbox begin name=SGR 1806 20Starbox image caption = This is where SGR 1806 20 would appear in the sky if it were visible to human eyes. Starbox observe epoch=J2000 ra=18h 08m 39.32s dec= 20° 24 39.5 appmag v= totally obscured… …

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  • 23Westerlund 1 — Cluster name = Westerlund 1 caption= Westerlund 1 epoch = J2000 class = Open cluster ra = RA|16|47|04.0 dec = DEC| 45|51|04.9 dist ly = 17.000 ly dist pc = 5214,72392638 pc appmag v = size v = mass kg = mass msol = radius ly = v hb = age =… …

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  • 24Subprime mortgage crisis — Part of a series on: Late 2000s financial crisis Major dimensions …

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  • 25CXO J164710.2-455216 — Starbox begin name=CXO J164710.2 455216 Starbox observe epoch=J2000.0 (ICRS) constell=Ara ra=RA|01|00|43.14 dec=DEC| 72|11|33.8 ! style= background color: #FFFFC0; colspan= 2 | Astrometry style= vertical align: top; Spectral type neutron star and …

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  • 26Westerlund 1 — Datos de observación (Época J2000.0) Tipo Supercúmulo estelar …

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  • 27Westerlund 1 — Datenbanklinks zu Westerlund 1 Offener Sternhaufen Westerlund 1 …

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  • 28Starquake —    A massive earthquake on a magnetar. A magnetar is a type of star that is created when a large star, at least eight times larger than the Sun, goes supernova. The star s core must spin fast, at least 200 revolutions per second, immediately… …

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  • 29Stellar magnetic field — A stellar magnetic field is a magnetic field generated by the motion of conductive plasma inside a main sequence (hydrogen burning) star. This motion is created through convection, which is a form of energy transport involving the physical… …

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  • 30Gamma ray burst progenitors — are the types of celestial objects that can emit gamma ray bursts (GRBs). GRBs show an extraordinary degree of diversity. They can last anywhere from a fraction of a second to many minutes. Bursts could have a single profile or oscillate wildly… …

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