2005MNRAS.360...76A

Query : 2005MNRAS.360...76A

2005MNRAS.360...76A - Mon. Not. R. Astron. Soc., 360, 76-80 (2005/June-2)

Σ-D relation for supernova remnants and its dependence on the density of the interstellar medium.

ARBUTINA B. and UROSEVIC D.

Abstract (from CDS):

During the last couple of decades of work on the Σ-D (radio surface brightness to diameter) relation for supernova remnants (SNRs), it has been generally accepted that no single Σ-D relation can be constructed for all SNRs. However, it may still be possible to construct the relations for some classes of SNRs. In our previous paper we analysed Σ-D relation(s) for remnants in the dense environments of molecular clouds. The aim of this paper is to examine, in the same context, a class of oxygen-rich SNRs, and to extend the analysis to remnants evolving in lower-density interstellar media, namely Balmer-dominated SNRs. We have obtained good relations with certain similarities to our previous findings - similarities that emphasize, again, the role of ambient density in the evolution of SNRs.

Abstract Copyright: 2005 RAS

Journal keyword(s): methods: statistical - supernova remnants - radio continuum: ISM

CDS comments: P.78 : IKT 19 is a misprint for IKT 25.

Simbad objects: 24

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Number of rows : 24
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 SN 1572A SN* 00 25 21.5 +64 08 27           B8 1254 1
2 V* S And No* 00 42 43.12368 +41 16 03.2124           ~ 190 2
3 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
4 SNR B0102-72.3 SNR 01 04 01.2 -72 01 52           ~ 422 1
5 MCSNR J0105-7223 SNR 01 05 05.6 -72 23 20           ~ 87 1
6 2E 273 XB* 01 06 19.49 -72 05 27.8     16.70     ~ 61 0
7 SNR B0505-67.9 SNR 05 05 42.0 -67 52 29           ~ 149 0
8 LHA 120-N 103B EmO 05 08 47.8 -68 45 39           ~ 244 1
9 SNR J050854-684447 SNR 05 08 59.26 -68 43 33.9           ~ 157 2
10 SNR B0509-67.5 SNR 05 09 31 -67 31.3           ~ 248 0
11 SNR B0519-69.0 SNR 05 19 35.14 -69 02 00.5           ~ 172 0
12 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
13 MCSNR J0525-6938 SNR 05 25 02.3 -69 38 39           ~ 446 1
14 NAME 30 Dor Nebula SFR 05 38 36.0 -69 05 11           ~ 1276 2
15 PSR B0540-69 Psr 05 40 11.2000490438 -69 19 54.198559829           ~ 976 3
16 SNR B0548-70.4 SNR 05 47 50.00 -70 24 54.0           ~ 91 0
17 NAME Pup A SNR 08 24 07 -42 59.8           ~ 636 1
18 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
19 SNR G292.0+01.8 SNR 11 24 59 -59 19.1           ~ 351 1
20 NGC 4449 EmG 12 28 11.118 +44 05 36.81 10.11 9.98 9.64 9.45   ~ 1192 1
21 NGC 5253 rG 13 39 55.990 -31 38 24.11 11.48 10.94 10.49 10.33 13.47 ~ 1421 4
22 NAME Lupus SN SNR 15 02 22.1 -42 05 49           ~ 1407 1
23 NAME Kepler's SN SNR 17 30 40.51 -21 29 14.4           ~ 851 3
24 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1

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