Zobrazeno 1 - 10
of 42
pro vyhledávání: '"E. B. Waltman"'
Publikováno v:
Symposium - International Astronomical Union. 219:181-186
Periodicities of radio flaring activity from the Algol systems β Per and δ Lib and the RS CVn systems V711 Tau and UX Ari were determined from a continuous 5-year survey. The radio continuum fluxes at 2.3 GHz and 8.3 GHz were monitored with the NRA
Publikováno v:
The Astrophysical Journal Supplement Series. 147:337-361
We report on the longest-running continuous radio flare survey of two Algol-type systems (β Per and δ Lib) and two RS CVn systems (V711 Tau and UX Ari). All four systems have late-type components, and all were known to display radio flaring activit
Autor:
Alan P. Marscher, J. Hallum, Margo F. Aller, Hugh D. Aller, H. Teräsranta, S. G. Jorstad, J. R. Mattox, E. B. Waltman
Publikováno v:
The Astrophysical Journal. 549:906-914
During the first 3 years of the Compton Gamma Ray Observatory mission, the blazar CTA 26 was observed 10 times by EGRET and not significantly detected. We report an observation in 1995 when CTA 26 flared to a peak γ-ray flux of (4.9 ± 1.5) × 10-6
Autor:
Sergei A. Trushkin, Rob Fender, Frank D. Ghigo, Robert M. Hjellming, Michael P. Rupen, Robert J. Sault, Richard W. Hunstead, Bryan Gaensler, Simon Garrington, Anita M. S. Richards, M. L. McCollough, D. Smith, C. J. de la Force, E. B. Waltman, D. Campbell-Wilson, A. J. Mioduszewski, Ralph Spencer
Publikováno v:
The Astrophysical Journal. 544:977-992
We report on radio observations of the 1999 September event of the X-ray transient V4641 Sgr (=XTE J1819-254=SAX J1819.3-2525). This event was extremely rapid in its rise and decay across radio, optical, and X-ray wavelengths; the X-rays rose to 12 c
Autor:
B. A. Harmon, Geoffrey N. Pendleton, R. S. Foster, S. N. Zhang, C. R. Robinson, Robert M. Hjellming, Frank D. Ghigo, K. J. Johnston, Michael L. McCollough, Michael S. Briggs, E. B. Waltman
Publikováno v:
The Astrophysical Journal. 517:951-955
Using CGRO/BATSE hard X-ray (HXR) data and GHz radio monitoring data from the Green Bank Interferometer (GBI), we have performed a long term study ($\sim$ 1800 days) of the unusual X-ray binary Cyg X-3 resulting in the discovery of a remarkable relat
Autor:
A. M. Stirling, T. W. B. Muxlow, Simon Garrington, Rob Fender, Ralph Spencer, Guy G. Pooley, E. B. Waltman, D. J. McKay
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 304, 865-876. Oxford University Press
We present high resolution MERLIN radio images of multiple relativistic ejections from GRS 1915+105 in 1997 October / November. The observations were made at a time of complex radio behaviour, corresponding to multiple optically-thin outbursts and se
Publikováno v:
The Astrophysical Journal. 507:371-383
We report dual circular polarization VLBA observations of Algol made at orbital phases 0.22-0.30 using a differential phase referencing technique. The flux density of Algol varied from 10 to 20 mJy during the observations. The radio maps show a doubl
Autor:
Shan-Jie Qian, Thomas P. Krichbaum, A. Witzel, Hugh D. Aller, Alexander Kraus, Silke Britzen, E. B. Waltman, E. Valtaoja
Publikováno v:
Chinese Astronomy and Astrophysics. 22:280-287
In this paper we use the “burst-injection model” of Qian et al. to analyze the evolution of the two mm-radio outbursts in 1991/93 in PKS 0528 + 134. comparison is made between the model and observed light curves at 12 frequencies between 230 GHz
Publikováno v:
The Astrophysical Journal. 491:381-387
LSI +61 303 is an exotic binary system consisting of a ~10 Msun B star and a compact object which is probably a neutron star. The system is associated with the interesting radio source GT0236+610 that exhibits bright radio outbursts with a period of
Publikováno v:
Vistas in Astronomy. 41:43-47
Quenching of the X-ray binary Cygnus X-3 at 2.25 GHz prior to outbursts during 1990–1993 is compared with published multi-frequency results. Flux density measurements obtained at 15 GHz with the Ryle Telescope during 1994–1995 are compared with f