THE CYGNUS X REGION .19. NO SUPERNOVA REMNANT IN THE W75 AREA

被引：1

作者：

WENDKER, HJ

HIGGS, LA

LANDECKER, TL

WARDTHOMPSON, D

机构：

[1] DOMINION RADIO ASTROPHYS OBSERV,PENTICTON V2A 6K3,BC,CANADA

[2] MULLARD RADIO ASTRON OBSERV,CAMBRIDGE CB3 0HE,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1993年 / 263卷 / 02期

关键词：

ISM-INDIVIDUAL-DR21; ISM-INDIVIDUAL-W75; ISM-SUPERNOVA REMNANTS;

D O I：

10.1093/mnras/263.2.543

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We point out that there is no observational evidence from existing radio data for a supernova remnant, recently suggested to exist, in the area of the source W75 (at approximately G81.6 + 1.0). Only a very unusual and hitherto unknown type of supernova remnant could have escaped detection. We further show that there is no compelling need to invoke a supernova remnant as the common cause of several radio features, since they are at different distances.

引用

页码：543 / 544

页数：2

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