Talk:LGM-1

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Suspicious numbers?[edit]

the numbers 1.337 and 420 both show up in this article? clever vandalism? I dunno ArmyOfFluoride (talk) 03:01, 21 January 2009 (UTC)[reply]

The period is 1.337302088331 s ^[1] (+/- 15 in the last two decimal places, if you care) The above ref also states approximate pulse widths of 28 milliperiods (at 10% of peak intensity) and 45 milliperiods (at 50%) By my calculation that is between 37 - 60 milliseconds. Also, this article contradicts PSR B1919+21 which gives "0.04 second" for the width. I'll change this article to 0.04 for now, since that agress with the ref. --mikeu ^talk 04:52, 21 January 2009 (UTC)[reply]

^ Arzoumanian, Z.; Nice, D. J.; Taylor, J. H.; Thorsett, S. E. (1994), "Timing behavior of 96 radio pulsars", Astrophysical Journal, 422 (2): 671, doi:10.1086/173760

Merge into PSR B1919+21 from LGM-1[edit]

The following discussion is closed. Please do not modify it. Subsequent comments should be made in a new section.

This should be merged to PSR B1919+21 —Preceding unsigned comment added by 90.179.235.249 (talk) 16:45, 5 May 2010 (UTC)[reply]

The above discussion is preserved as an archive. Please do not modify it. Subsequent comments should be made in a new section.

[Arzoumanian1994-1] Arzoumanian, Z.; Nice, D. J.; Taylor, J. H.; Thorsett, S. E. (1994), "Timing behavior of 96 radio pulsars", Astrophysical Journal, 422 (2): 671, doi:10.1086/173760

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