Timing analysis of the core of the Crab-like SNR G21.5–0.9

Publisher： Edp Sciences

E-ISSN： 1432-0746|383|3|916-918

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.383, Iss.3, 2002-03, pp. : 916-918

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

The extended X-ray halo of the Crab-like SNR G21.5-0.9

By  

Astronomy & Astrophysics, Vol. 365, Iss. 1, 2001-01 ,pp. : L248-L253

Edp Sciences

Access to resources Recommend Favorite

Infrared imaging and polarimetric observations of the pulsar wind nebula in SNR G21.5-0.9

By Zajczyk A.   Gallant Y. A.   Slane P.   Reynolds S. P.   Bandiera R.   Gouiffès C.   Le Floc’h E.   Comerón F.   Koch Miramond L.  

Astronomy & Astrophysics, Vol. 542, Iss. issue, 2012-05 ,pp. : A12-A12

Edp Sciences

Access to resources Recommend Favorite

On particle acceleration and very high energy $\gamma$-ray emission in Crab-like pulsars

By  

Astronomy & Astrophysics, Vol. 502, Iss. 1, 2009-07 ,pp. : 15-20

Edp Sciences

Access to resources Recommend Favorite

XMM-Newton spectral analysis of the Pulsar Wind Nebula within the composite SNR G0.9+0.1

By  

Astronomy & Astrophysics, Vol. 401, Iss. 1, 2003-04 ,pp. : 197-203

Edp Sciences

Access to resources Recommend Favorite

Discovery of a new faint radio SNR G108.2-0.6

By  

Astronomy & Astrophysics, Vol. 465, Iss. 3, 2007-04 ,pp. : 907-911

Edp Sciences

Access to resources Recommend Favorite