Pulsar microstructure and its quasi-periodicities withthe S2 VLBI system at a resolution of 62.5 nanoseconds

E-ISSN： 1432-0746|396|1|171-187

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.396, Iss.1, 2002-12, pp. : 171-187

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

Quasi-periodicities of BL Lacertae objects

By Sandrinelli A. Covino S. Treves A. Holgado A. M. Sesana A. Lindfors E. Ramazani V. F.

Astronomy & Astrophysics, Vol. 615, Iss. issue, 2018-07 ,pp. : A118-A118

Edp Sciences

Access to resources Recommend Favorite

Orbital evolution of colliding star and pulsar winds in 2D and 3D: effects of dimensionality, EoS, resolution, and grid size

By Bosch-Ramon V. Barkov M. V. Perucho M.

Astronomy & Astrophysics, Vol. 577, Iss. issue, 2015-05 ,pp. : A89-A89

Edp Sciences

Access to resources Recommend Favorite

The very long baseline interferometry (VLBI) system’s unfinished business.

By Phipps Jr.

Physics Essays, Vol. 23, Iss. 1, 2010-03 ,pp. : 206-208

Physics Essays Publication

Access to resources Recommend Favorite

Phenomenology of pulsar B0809+74's rotating subbeam system

Astronomy & Astrophysics, Vol. 455, Iss. 1, 2006-08 ,pp. : 215-221

Edp Sciences

Access to resources Recommend Favorite

Phenomenology of pulsar B0809+74's rotating subbeam system

Astronomy & Astrophysics, Vol. 447, Iss. 1, 2006-02 ,pp. : 235-243

Edp Sciences

Access to resources Recommend Favorite