The radio counterpart of the likely TeV binary HESS J0632+057
نویسندگان
چکیده
منابع مشابه
The radio counterpart of the likely TeV binary HESSJ 0632 + 057
The few known γ-ray binary systems are all associated with variable radio and Xray emission. The TeV source HESS J0632+057, apparently associated with the Be star MWC148, is plausibly a new member of this class. Following the identification of a variable X-ray counterpart to the TeV source we conducted GMRT and VLA observations in June-September 2008 to search for the radio counterpart of this ...
متن کاملA Radio Counterpart for the Unidentified Tev Source Hess J1813-178: the Radio-gamma-ray Connection
We discovered independently the shell-type supernova remnant G12.82−0.02, recently reported by Brogan et al. (2005), which is coincident with the unidentified TeV gamma-ray source revealed in the HESS survey of the Galactic plane. Estimating the ambient starlight at the location of this source from the integrated Lyα luminosity of the nearby H II region W33, we conclude that inverse Compton emi...
متن کاملDiscovery of the Radio and X-ray Counterpart of Tev Γ-ray Source Hess J1731-347
We discover a faint shell-type radio and X-ray source, G353.6-0.7, associated with HESS J1731-347. G353.6-0.7 is likely an old supernova remnant (SNR), based on radio (0.8 GHz, 1.4 GHz and 5 GHz), infrared (8 µm from the GLIMPSE Legacy Project and 21 µm from the Midcourse Space Experiment), and X-ray (0.1 keV-2.4 keV from the ROSAT survey and 5-20 keV from the INTEGRAL survey) data. The SNR, ce...
متن کاملIdentification of a Likely Radio Counterpart of the Rapid Burster
We have identified a likely radio counterpart to the low-mass X-ray binary MXB 1730−335 (the Rapid Burster). The counterpart has shown 8.4 GHz radio on/off behavior correlated with the X-ray on/off behavior as observed by the RXTE/ASM during six VLA observations. The probability of an unrelated, randomly varying background source duplicating this behavior is 1–3% depending on the correlation ti...
متن کاملIdentification of a Likely Radio Counterpart to the Rapid Burster
We have identiÐed a likely radio counterpart to the low-mass X-ray binary MXB 1730[335 (the Rapid Burster). The counterpart has shown 8.4 GHz radio on/o† behavior correlated with the X-ray on/o† behavior as observed by the RXT E/ASM during six VLA observations. The probability of an unrelated, randomly varying background source duplicating this behavior is 1%È3% depending on the correlation tim...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2009
ISSN: 0035-8711,1365-2966
DOI: 10.1111/j.1365-2966.2009.15272.x