Talk:LGM-1

This redirect is within the scope of WikiProject Astronomy, which collaborates on articles related to Astronomy on Wikipedia.AstronomyWikipedia:WikiProject AstronomyTemplate:WikiProject AstronomyAstronomy

History of Science

This redirect is part of the History of Science WikiProject, an attempt to improve and organize the history of science content on Wikipedia. If you would like to participate, you can edit the redirect attached to this page, or visit the project page, where you can join the project and/or contribute to the discussion. You can also help with the History of Science Collaboration of the Month.History of ScienceWikipedia:WikiProject History of ScienceTemplate:WikiProject History of Sciencehistory of science

Telecommunications

This redirect is within the scope of WikiProject Telecommunications, a collaborative effort to improve the coverage of Telecommunications on Wikipedia. If you would like to participate, please visit the project page, where you can join the discussion and see a list of open tasks.TelecommunicationsWikipedia:WikiProject TelecommunicationsTemplate:WikiProject TelecommunicationsTelecommunications

Suspicious numbers?

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

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

[1]