RADIO SUPERNOVAE

[1] AKSENOV EP, 1981, IAU3580 CIRC

[2] AKSENOV EP, 1984, IAU3907 CIRC

[3] ALLEN RJ, 1976, ASTRON ASTROPHYS, V48, P253

[4] ARGYLE RW, 1984, IAU3985 CIRC

[5] ARGYLE RW, 1984, IAU3912 CIRC

[6] TYPE-I SUPER-NOVAE .1. ANALYTIC SOLUTIONS FOR THE EARLY PART OF THE LIGHT-CURVE [J]. ASTROPHYSICAL JOURNAL, 1982, 253 (02) : 785 - 797

[7] BANDIERA R, 1983, ASTRON ASTROPHYS, V126, P7

[8] THE EVOLUTION OF NONTHERMAL SUPERNOVA-REMNANTS .2. CAN RADIO SUPERNOVAE BECOME PLERIONS [J]. ASTROPHYSICAL JOURNAL, 1984, 285 (01) : 134 - 140

[9] BARBON R, 1982, ASTRON ASTROPHYS, V116, P35

[10] Barbon R., 1984, Astronomy & Astrophysics Supplement Series, V58, P735

[1] AKSENOV EP, 1981, IAU3580 CIRC

[2] AKSENOV EP, 1984, IAU3907 CIRC

[3] ALLEN RJ, 1976, ASTRON ASTROPHYS, V48, P253

[4] ARGYLE RW, 1984, IAU3985 CIRC

[5] ARGYLE RW, 1984, IAU3912 CIRC

[6] TYPE-I SUPER-NOVAE .1. ANALYTIC SOLUTIONS FOR THE EARLY PART OF THE LIGHT-CURVE [J]. ASTROPHYSICAL JOURNAL, 1982, 253 (02) : 785 - 797

[7] BANDIERA R, 1983, ASTRON ASTROPHYS, V126, P7

[8] THE EVOLUTION OF NONTHERMAL SUPERNOVA-REMNANTS .2. CAN RADIO SUPERNOVAE BECOME PLERIONS [J]. ASTROPHYSICAL JOURNAL, 1984, 285 (01) : 134 - 140

[9] BARBON R, 1982, ASTRON ASTROPHYS, V116, P35

[10] Barbon R., 1984, Astronomy & Astrophysics Supplement Series, V58, P735