Jet interaction of SS 433 with the ambient medium

被引：8

作者：

Durouchoux, P ^{[1
]}

Sood, R

Oka, T

Segers, M

Safi-Harb, S

Vilhu, O

Huovelin, J

Thresher, D

Corbel, S

O'Neill, P

机构：

[1] CE Saclay, DSM, DAPNIA, Serv Astrophys, F-91191 Gif Sur Yvette, France

[2] Univ New S Wales, Univ Coll, ADFA, Sch Phys, Canberra, ACT 2600, Australia

[3] RIKEN, Wako, Saitama 35101, Japan

[4] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA

[5] Univ Helsinki, Observ Helsinki, FIN-00014 Helsinki, Finland

[6] Ecole Cent Paris, F-92295 Chatenay Malabry, France

来源：

BROAD BAND X-RAY SPECTRA OF COSMIC SOURCES | 2000年 / 25卷 / 3-4期

关键词：

D O I：

10.1016/S0273-1177(99)00826-1

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

SS 433 is a bright X-ray binary with two sided jets moving at 0.26 c. It is located at the center of the supernova remnant W50, suggesting that SS 433 is associated with W50. A large molecular cloud also surrounds the SS 433/W50 system. Recent observations with ROSAT and ASCA have shown X-ray hot spots interpreted as SS 433 jets interacting with the ambient interstellar medium. To verify this hypothesis, we have performed observations of the molecular cloud around SS 433 in the J = 1-0 and J = 2-1 lines of CO transitions along and perpendicular to the jet axis and have found two clouds with velocities of 32 km/s and 50 km/s respectively. Due to a strong correlation between the 50 km/s map and the X-ray hot spots, we conclude that SS 433 is inside or at the edge of the 50 km/s molecular cloud. (C) 2000 COSPAR. Published by Elsevier Science Ltd.

引用

页码：703 / 708

页数：6

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