Radio images of the microquasar GRS 1758-258

被引：32

作者：

Martí, J

Mirabel, IF

Rodríguez, LF

Smith, IA

机构：

[1] Univ Jaen, Escuela Politecn Super, Dept Fis, Jaen, Spain

[2] CSIC, Inst Astrofis Andalucia, Granada, Spain

[3] Ctr Etud Saclay, Serv Astrophys, CEA, DSM,DAPNIA, F-91191 Gif Sur Yvette, France

[4] Inst Astron & Fis Espacio, RA-1428 Buenos Aires, DF, Argentina

[5] Univ Nacl Autonoma Mexico, Inst Astron, Morelia 58089, Michoacan, Mexico

[6] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA

来源：

ASTRONOMY & ASTROPHYSICS | 2002年 / 386卷 / 02期

关键词：

stars : individual : GRS 1758-258; stars; winds; outflows;

D O I：

10.1051/0004-6361:20020273

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present sensitive images of the microquasar GRS 1758-258 at two different radio wavelengths. The positions, flux densities and spectral indices of the central source and the extended radio lobes are reported. Our results confirm the synchrotron nature of the radio lobes. We also present a very deep radio image of the jet flow at arcminute scales. The source VLA-C, previously proposed as the exciting source of the system, is found to coincide with the Chandra position.

引用

页码：571 / 575

页数：5

共 16 条

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CASTROTIRADO AJ, 2001, AP SS, P276

[2] Deep infrared imaging of the microquasars 1E 1740-2942 and GRS 1758-2581 [J].