Simultaneous multi-wavelength observations of GRS 1915+105

被引:51
作者
Fuchs, Y [1 ]
Rodriguez, J
Mirabel, IF
Chaty, S
Ribó, M
Dhawan, V
Goldoni, P
Sizun, P
Pooley, GG
Zdziarski, AA
Hannikainen, DC
Kretschmar, P
Cordier, B
Lund, N
机构
[1] CEA Saclay, Serv Astrophys, CNRS, FRE 2591, F-91191 Gif Sur Yvette, France
[2] Integral Sci Data Ctr, CH-1290 Versoix, Switzerland
[3] Consejo Nacl Invest Cient & Tecn, Inst Astron & Fis Espacio, RA-1428 Buenos Aires, DF, Argentina
[4] Univ Paris 07, Federat APC, F-75005 Paris, France
[5] Natl Radio Astron Observ, Socorro, NM 87801 USA
[6] Univ Cambridge, Cavendish Lab, Mullard Radio Astron Observ, Cambridge CB3 0HE, England
[7] Nicholas Copernicus Astron Ctr, PL-00716 Warsaw, Poland
[8] Univ Helsinki Observ, Helsinki 00014, Finland
[9] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[10] Danish Space Res Inst, DK-2100 Copenhagen OE, Denmark
关键词
stars : individual : GRS 1915+105; X-rays : binaries; gamma rays : observations; ISM : jets and outflows; X-RAY STATES; GRS 1915+105; RADIO-EMISSION; SUPERLUMINAL SOURCE; GALAXY; COMPTONIZATION; JETS;
D O I
10.1051/0004-6361:20031338
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the result of multi-wavelength observations of the microquasar GRS 1915 + 105 in a plateau state with a luminosity of similar to7.5 x 10(38) erg s(-1) (similar to40% L-Edd), conducted simultaneously with the INTEGRAL and RXTE satellites, the ESOstarstar/NTT, the Ryle Telescope, the NRAO(starstarstar) VLA and VLBA, in 2003 April 2-3. For the first time were observed concurrently in GRS 1915 + 105 all of the following properties: a strong steady optically thick radio emission corresponding to a powerful compact jet resolved with the VLBA, bright near-IR emission, a strong QPO at 2.5 Hz in the X-rays and a power law dominated spectrum without any cutoff in the 3-400 keV range.
引用
收藏
页码:L35 / L39
页数:5
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