J1856
  Home FAQ Contact Sign in
 
Advanced search
MATCHING GROUPS



more...
POPULAR GROUPS

more...

found 2 articles for 0.303 sec
>From Osher Doctorow C. Motch of Observatoire Astronomique Strasbourg (U. Strasbourg) France and W. C. G. Ho of Harvard-Smithsonian CfA in separate papers, and their colleagues, have indicated scenarios in which emitting properties of the surface of the Strange Star candidate RX J 1856.5-3754 could account for this being a Strange Star. See Motch, C., Zavlin, V. E., Haberl F., A&A 408, 303     

Group: sci.physics · Group Profile · Search for J1856 in sci.physics
Author: OsherD
Date: Jun 1, 2007 22:39

ESA News http://www.esa.int 9 March 2007 XMM-Newton finds the leader of the Magnificent Seven in a spin A decade-long mystery has been solved using data from ESA's X-ray observatory XMM-Newton. The brightest member of the so-called 'magnificent seven' has been found to pulsate with a period of seven seconds. The discovery casts some doubt on the recent interpretation that this object
Show full article (2.12Kb)
    

Group: sci.space.news · Group Profile · Search for J1856 in sci.space.news
Author: Andrew Yee
Date: Mar 13, 2007 15:31

Show full article (4.28Kb)