1984ApJ...285..134B

Query : 1984ApJ...285..134B

1984ApJ...285..134B - Astrophys. J., 285, 134-140 (1984)

The evolution of nonthermal supernova remnants. II. Can radio supernovae become plerions ?

BANDIERA R., PACINI F. and SALVATI M.

Journal keyword(s):

Errata: + erratum vol. 291, 394

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
2 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
3 NAME Vela X Psr 08 33 08.880 -45 11 24.36           ~ 302 1
4 SN 1979C SN* 12 22 58.58 +15 47 52.7   11.6       SNIIL 609 1
5 SN 1957D SN* 13 37 03.57 -29 49 40.7   15.0 15.0     ~ 121 1
6 SN 1970G SN* 14 03 00.83 +54 14 32.8   11.8 11.50     SNIIL 221 1
7 SN 1981J SN* 14 03 17 +38 31.5   15.0 15.0     SNI 8 1
8 SN 1980K SN* 20 35 30.07 +60 06 23.7   11.6       SNIIL 482 1

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