Field approach to gravitation and its significance in astrophysics Vladimír Majerník OriginalPaper Pages: 265 - 285
Radio emission of galactic clusters at 1.4 GHz and 2.7 GHz R. Schwartz OriginalPaper Pages: 286 - 300
The energy spectrum of primary cosmic ray electrons from 2 GeV to 200 GeV J. L. FanselowR. C. HartmanP. J. Schmidt OriginalPaper Pages: 301 - 313
On the dependence ofQ metallicity index from basic parameters of stellar evolution Francesca A. D'Antona OriginalPaper Pages: 314 - 316
Excitation of O2 Herzberg Bands in the nightglow R. D. SrivastavaR. V. ShuklaA. N. Srivastava OriginalPaper Pages: 317 - 322
On the evolutionary stage of stars in the Draco dwarf Galaxy Filippina CaputoVittorio Castellani OriginalPaper Pages: 323 - 331
Implosions and emplosions in supermassive objects Giora ShavivGerald E. Tauber OriginalPaper Pages: 396 - 398
On the modulation and energy spectrum of highly charged cosmic ray nuclei T. F. CleghornPhyllis S. FreierC. J. Waddington OriginalPaper Pages: 422 - 430
Variation of the gradient and balmer discontinuity during the eclipse of the variable RW Tauri: Comparison between observations and theory Pier Luigi BattistiniMassimo FracassiniLaura E. Pasinetti OriginalPaper Pages: 438 - 445
The ordinary URCA process in the presence of positrons and large magnetic fields Ronald W. McFee OriginalPaper Pages: 446 - 453
Exact cosmological solutions in Brans and Dicke's scalar-tensor theory, I H. DehnenO. Obregón OriginalPaper Pages: 454 - 459
Infra-red emission from galactic nuclei Krishna M. V. ApparaoT. N. Rengarajan OriginalPaper Pages: 460 - 463
Magnetic stars with an external non-linear force-free field M. A. Raadu OriginalPaper Pages: 464 - 472
Cosmic flux of low energy gamma rays S. V. DamleR. R. DanielP. J. Lavakare OriginalPaper Pages: 473 - 479
Observations of the planetary nebula NGC 6853 at [Nii] 6584 Å A. C. Danks OriginalPaper Pages: 480 - 484
A possible mechanism for the injection of particles into a cosmic ray acceleration region K. Kristiansson OriginalPaper Pages: 485 - 500