Are Pulsars Born as Slow Rotators? |
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Page 24
... Seward et al . ( 1983 ) and the distance to PSR 0833-45 ( Vela ) is from Seward ( 1983 ) . The two sources around the Vela pulsar are a small one of size 1 ' x 0.8 ' ( A ) and a more extended one of size 30 ' x 60 ' ( B ) ( Seward 1983 ) ...
... Seward et al . ( 1983 ) and the distance to PSR 0833-45 ( Vela ) is from Seward ( 1983 ) . The two sources around the Vela pulsar are a small one of size 1 ' x 0.8 ' ( A ) and a more extended one of size 30 ' x 60 ' ( B ) ( Seward 1983 ) ...
Page 29
... Seward et al . 1983 . 4. Seward 1983 . 5. Helfand 1983 . 6 . Cheng 1984 . REFERENCES · Becker , R. H. , Helfand , D. 29.
... Seward et al . 1983 . 4. Seward 1983 . 5. Helfand 1983 . 6 . Cheng 1984 . REFERENCES · Becker , R. H. , Helfand , D. 29.
Page 31
... Seward , F. D. 1983 , in I.A.U. Symposium No. 101 , Supernova Remnants and Their X - Ray Emission , ed . J. Danziger and P. Gorenstein ( Dordrecth : Reidel ) , p . 405 . Seward , F. D. , Harnden , F. R. , Mudrin , P. , and Clark , D. H. ...
... Seward , F. D. 1983 , in I.A.U. Symposium No. 101 , Supernova Remnants and Their X - Ray Emission , ed . J. Danziger and P. Gorenstein ( Dordrecth : Reidel ) , p . 405 . Seward , F. D. , Harnden , F. R. , Mudrin , P. , and Clark , D. H. ...
Contents
DISTRIBUTION PERPENDICULAR TO THE GALACTIC PLANE | 14 |
SYNCHROTRON NEBULAE AROUND PULSARS | 23 |
DISCUSSION | 26 |
Common terms and phrases
approximately assumed assumption average calculated Cheng choosing compact compared complete consider consistent constant curve derived determined difference distance distribution of pulsars effect emission energy equation equation 11 error estimate expected factor Figure flux function galactic plane given gives Gobs Gunn and Ostriker height Helfand implies indicated initial period integrated less limit luminosity Lyne magnetic dipole magnetic field Manchester and Taylor measured nebulae normalized observed distribution observed pulsars obtain parameters period distribution perpendicular possible present probability properties pulsars are born radio luminosity range Reynolds rotation sample scale height seen sensitive Seward shown in Figure similar smaller standard model suggest supernova remnants survey tion typical uncertainties v₂ values variables variation velocity distribution Vivekenand and Narayan x-ray