Interaction between the interstellar medium and solar wind plasma Max K. Wallis OriginalPaper Pages: 3 - 18
Comments on the paper by Mack and Robbins relating to a recent theory on the origin of the universal X-ray background P. RaychaudhuriP. Bandyopadhyay Research Note Pages: 43 - 44
On a recent theory of the origin of the X-ray backgroun-dfurther arguments: Comments on the preceding note John E. MackDonald E. Robbins Research Note Pages: 45 - 46
Ultrahigh energy photons, electrons, and neutrinos, the microwave background, and the universal cosmic-ray hypothesis F. W. Stecker OriginalPaper Pages: 47 - 57
On a possible mechanism responsible for the differential energy spectrum of relativistic electrons and non-linear low-frequency spectra of cosmic radio sources S. Ya. BraudeÈ. A. Kaner OriginalPaper Pages: 59 - 70
Energy spectrum of HeII in a strong magnetic field and bound-bound transition probabilities G. L. SurmelianR. F. O'Connell OriginalPaper Pages: 85 - 91
The spectrum of RR Telescopii in 1968 L. H. AllerR. S. PolidanGordon W. Wares OriginalPaper Pages: 93 - 110
A reappraisal of several extensive phenomena of the high galactic latitudes K. H. ElliottJ. Meaburn OriginalPaper Pages: 111 - 122
The synthesis of close-binary light curves IV: An application to TX ursae majoris and MR Cygni Graham HillJ. B. Hutchings OriginalPaper Pages: 123 - 148
A two-beam, multi-mode, nebular-stellar photometer C. GoudisJ. Meaburn OriginalPaper Pages: 149 - 157
Energy losses of galactic cosmic rays in the interplanetary medium I. H. UrchL. J. Gleeson OriginalPaper Pages: 177 - 185
The effects of stark broadening in the radio recombination line temperatures Janet P. Simpson OriginalPaper Pages: 187 - 203
Extinction and scattering by several types of silicate sphere of radius 0.05–1.0μm, for the wavelength range 0.21–50μm G. E. BromageK. NandyB. N. Khare OriginalPaper Pages: 213 - 224
Temperature dependent nuclear mass and its application to astrophysical problems Teruaki Ohnishi OriginalPaper Pages: 225 - 239
187Re, recyclingR-process elements through stars, and the age of the Galaxy Raymond J. Talbot Jr. OriginalPaper Pages: 241 - 249
Test for detection of fine structure of the solar wind velocity N. A. LotovaI. V. Chashey OriginalPaper Pages: 251 - 262