Cosmic rays and the Monogem supernova remnant

[1]  K. Yoshida,et al.  The Most Likely Sources of High-Energy Cosmic-Ray Electrons in Supernova Remnants , 2003, astro-ph/0308470.

[2]  M. Roth,et al.  Energy spectrum and mass composition of high-energy cosmic rays , 2003 .

[3]  A. Erlykin,et al.  High-energy cosmic gamma rays from the 'single source' , 2003, astro-ph/0302380.

[4]  A. Erlykin,et al.  Supernova remnants and the origin of cosmic radiation: evidence from low-energy gamma rays , 2002 .

[5]  A. Erlykin,et al.  Ultra high energy cosmic rays and pulsars , 2002 .

[6]  A. Erlykin,et al.  Supernova remnants and the origin of the cosmic radiation: the electron component , 2002 .

[7]  A. Erlykin,et al.  Supernova remnants and the origin of the cosmic radiation: I. SNR acceleration models and their predictions , 2001 .

[8]  A. Erlykin,et al.  Structure in the cosmic ray spectrum: an update , 2001 .

[9]  A. Erlykin,et al.  A single source of cosmic rays in the range - eV , 1997 .

[10]  D. McCammon,et al.  ROSAT Survey Observations of the Monogem Ring , 1996 .

[11]  E. Phinney,et al.  Binary and Millisecond Pulsars , 1994 .

[12]  A. Erlykin,et al.  Energy dependence of the mass composition of primary cosmic rays in the 1-10 PeV energy interval , 1993 .

[13]  C. Fichtel,et al.  High-energy and ultra-high-energy cosmic rays , 1986 .

[14]  J. Nousek,et al.  The Gemini-Monoceros X-ray enhancement - A giant X-ray ring , 1981 .

[15]  V. Blobel,et al.  Inclusive neutron and lambda production in proton-proton interactions at 12 and 24 GeV/c , 1978 .