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Simultaneous Multi-Wavelength Observations of Microquasars (The Mine Collaboration)

Published online by Cambridge University Press:  22 February 2018

Y. Fuchs ,
J. Rodriguez ,
I. F. Mirabel ,
S. E. Shaw ,
P. Kretschmar ,
M. Ribó ,
S. Chaty ,
V. Dhawan ,
I. Brown  and
R. Spencer
...Show all authors
Y. Fuchs
Affiliation:
Service d'Astrophysique, CEA/Saclay, France
J. Rodriguez
Affiliation:
Service d'Astrophysique, CEA/Saclay, France INTEGRAL Science Data Center, Versoix, Switzerland
I. F. Mirabel
Affiliation:
Service d'Astrophysique, CEA/Saclay, France
S. E. Shaw
Affiliation:
INTEGRAL Science Data Center, Versoix, Switzerland University of Southampton, Southampton, UK
P. Kretschmar
Affiliation:
INTEGRAL Science Data Center, Versoix, Switzerland MPE, Garching, Germany
M. Ribó
Affiliation:
Service d'Astrophysique, CEA/Saclay, France
S. Chaty
Affiliation:
Service d'Astrophysique, CEA/Saclay, France Université Paris 7, Paris, France
V. Dhawan
Affiliation:
National Radio Astronomy Observatory, SocorroUSA
I. Brown
Affiliation:
Jodrell Bank, Manchester Univ., UK
R. Spencer
Affiliation:
Jodrell Bank, Manchester Univ., UK
G. G. Pooley
Affiliation:
Mullard Radio Astronomy Obs., Cambridge, UK
D. C. Hannikainen
Affiliation:
University of Helsinki, Helsinki, Finland

Abstract

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We present the international collaboration MINE (Multi-λ INTEGRAL NEtwork) aimed at conducting multi wavelength observations of microquasars simultaneously with the INTEGRAL satellite. The first results of GRS 1915+105 are encouraging and those to come should help us to understand the physics of the accretion and ejection phenomena around a compact object.

Resumen

Resumen

Presentamos la colaboración internacional MINE (Multi-λ INTEGRA NEtwork) cuya meta es llevar a cal observaciones en múltiples longitudes de onda de microcuasares de forma simultánea al satélite INTEGRA Los primeros resultados con GRS 1915+105 son muy esperanzadores y junto con los que se obtendrán en futuro nos ayudarán a comprender la física de los fenómenos de acreción y eyección relacionados con los sistem binarios compactos.

Keywords

StarsIndividual (GRS 1915+105) — X-RaysBinaries
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 28 - 29
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Dhawan, V., Mirabel, I. F., & Rodríguez, L. F. 2000 ApJ, 543, 373 Google Scholar
Fender, R. P., Garrington, S. T., McKay, D. J., et al 1999, MNRAS, 304, 865 CrossRefGoogle Scholar
Fuchs, Y., Mirabel, I. F. & Claret, A. 2003a, A&A, 404, 1011 Google Scholar
Fuchs, Y., Rodríguez, J., Mirabel, I. F., et al. 2003b A&A, 409, L35 Google Scholar
Greiner, J., Cuby, J. G. & McCaughrean, M. J. 2001 Nature, 414, 522 CrossRefGoogle Scholar
McClintock, J. E. & Remillard, R. A. 2004, in ‘Compac Stellar X-Ray Sources', eds. Lewin, W.H.G. and Klis, M. van der, CUP, astro-ph/0306213Google Scholar
Mirabel, I. F. & Rodríguez, L. F. 1994, Nature, 371, 46 Google Scholar
Mirabel, I. F. & Rodríguez, L. F. 1999, ARA&A, 37, 40 Google Scholar
Rodríguez, J., Hannikainen, D., et al. 2004, this volumeGoogle Scholar
Zdziarski, A. A., Grove, J. E., Poutanen, J., et al. 2003 ApJ, 554, L45 CrossRefGoogle Scholar