21 research outputs found
MERLIN observations of GRS 1915+105 : a progress report
We present a progress report on MERLIN radio imaging of a radio outburst from
GRS 1915+105. The major ejection occurred at the end of an approximately 20-day
`plateau' state, characterised by low/hard X-ray fluxes and a relatively strong
flat-spectrum radio component. Apparent superluminal motions have been mapped
with unprecedented resolution, and imply higher velocities in the jet than
previously derived.Comment: 4 pages, 2 figures. To be published in New Astronomy Reviews, as part
of proceedings of 2nd workshop on Galactic sources with relativistic jet
Light curves and radio structure for the September 1999 transient event in XTE J1819-254 (=SAX J1819.3-2325 = V4641 Sagittarii)
A High Statistics Search for Ultra-High Energy Gamma-Ray Emission from Cygnus X-3 and Hercules X-1
We have carried out a high statistics (2 Billion events) search for
ultra-high energy gamma-ray emission from the X-ray binary sources Cygnus X-3
and Hercules X-1. Using data taken with the CASA-MIA detector over a five year
period (1990-1995), we find no evidence for steady emission from either source
at energies above 115 TeV. The derived upper limits on such emission are more
than two orders of magnitude lower than earlier claimed detections. We also
find no evidence for neutral particle or gamma-ray emission from either source
on time scales of one day and 0.5 hr. For Cygnus X-3, there is no evidence for
emission correlated with the 4.8 hr X-ray periodicity or with the occurrence of
large radio flares. Unless one postulates that these sources were very active
earlier and are now dormant, the limits presented here put into question the
earlier results, and highlight the difficulties that possible future
experiments will have in detecting gamma-ray signals at ultra-high energies.Comment: 26 LaTeX pages, 16 PostScript figures, uses psfig.sty to be published
in Physical Review
Magnetic field estimation in Cyg X-3’s jet
Multi-wavelength photometric observations of Cygnus X-3 were carried out at 18 cm through to 450 µm, complemented by X-ray (2-10 keV) observations. The system was mildly active with cm fluxes at 150 – 250 mJy. We find the spectrum to be flat with a spectral index of zero. Using a modified Wolf-Rayet wind model, and assuming emission is generated in synchrotron emitting jets from the source, we find an upper-limit to the magnetic field of 20 G at a distance 5×10 12 cm is required. 1