INTEGRAL and XMM-Newton observations towards the unidentified MeV source GRO J1411-64

• Autores: Torres, Diego F.; Zhang, S.; Reimer, O.; Barcons, X.; Corral, A.; Bosch Ramon, Valentí; Paredes, Josep Maria; Romero, Gustavo Esteban; Qu, J. L.; Collmar, W.; Schönfelder, V.; Butt, Y.
• Año de publicación: 2006
• Idioma: inglés
• Tipo de recurso: artículo
• Materia: X-rays; Gamma rays; Gamma ray observations
• Institución: Consejo Nacional de Investigaciones Científicas y Técnicas

Aims. We investigate the nature of the COMPTEL unidentified source GRO J1411-64. Methods. The source was observed by INTEGRAL. Its central part was also observed by XMM-Newton. Results. The data analysis shows no hint for new detections at hard X-rays. The upper limits in flux herein presented constrain the energy spectrum of whatever was producing GRO J1411-64, imposing, in the framework of earlier COMPTEL observations, the existence of a peak in power output located somewhere between 300–700 keV for the so-called low state. The Circinus Galaxy is the only source detected within the 4σ location error of GRO J1411-64, but can be safely excluded as the possible counterpart: the extrapolation of the energy spectrum is well below the one for GRO J1411-64 at MeV energies. 22 reliable and statistically significant sources (likelihood > 10) were extracted and analyzed from XMM-Newton data. Only one of these sources, XMMU J141255.6-635932, is spectrally compatible with GRO J1411-64 although the fact the soft X-ray observations do not cover the full extent of the COMPTEL source position uncertainty make an association hard to quantify and thus risky. Conclusions. The unique peak of the power output at high energies (hard X-rays and gamma-rays) resembles that found in the SED seen in blazars or microquasars, and might suggest that a similar scenario is at work. However, an analysis using a microquasar model consisting on a magnetized conical jet filled with relativistic electrons which radiate through synchrotron and inverse Compton scattering with star, disk, corona and synchrotron photons shows that it is hard to comply with all observational constrains. This fact and the non-detection at hard X-rays introduce an a-posteriori question mark upon the physical reality of this source, which is discussed in some detail
Fil: Torres, Diego F.. Institut de Ciències de l’Espai; España
Fil: Zhang, S.. Institute of High Energy Physics. Laboratory for Particle Astrophysics; China
Fil: Reimer, O.. Stanford University; Estados Unidos
Fil: Barcons, X.. Instituto de Física de Cantabria; España
Fil: Corral, A.. Instituto de Física de Cantabria; España
Fil: Bosch Ramon, Valentí. Universidad de Barcelona; España
Fil: Paredes, Josep Maria. Universidad de Barcelona; España
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
Fil: Qu, J. L.. Institute of High Energy Physics. Laboratory for Particle Astrophysics; China
Fil: Collmar, W.. Max Planck Institut für extraterrestrische Physik; Alemania
Fil: Schönfelder, V.. Max Planck Institut für extraterrestrische Physik; Alemania
Fil: Butt, Y.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos