Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7−3946
نویسندگان
چکیده
منابع مشابه
Prospects for Cherenkov Telescope Array Observations of the Young Supernova
We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX J1713.7−3946, a young supernova remnant (SNR) and one of the brightest sources ever discovered in very-high-energy (VHE) gamma rays. Special attention is paid to explore possible spatial (anti-)correlations of gamma rays with emission at other wavelengths, in particular X-rays and CO/Hi emission. We present a s...
متن کاملCangaroo-iii Observations of the Supernova Remnant Rx J0852.0−4622
Sub-TeV gamma-ray emission from the North-West rim of the supernova remnant RX J0852.0−4622 was detected with the CANGAROO-II telescope and recently confirmed by the H.E.S.S. group. In addition, the H.E.S.S. data revealed a very wide (up to two degrees in diameter), shell-like profile of the gamma-ray emission. We have carried out CANGAROO-III observations in January and February 2005 with thre...
متن کاملGamma-ray Observations of the Supernova Remnant Rx J0852.0−4622 with the Fermi Lat
We report on gamma-ray observations of the supernova remnant (SNR) RX J0852.0−4622 with the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope. In the Fermi LAT data, we find a spatially extended source at the location of the SNR. The extension is consistent with the SNR size seen in other wavelengths such as X-rays and TeV gamma rays, leading to the identification of the gam...
متن کاملXMM - Newton observations of the supernova remnant RX J 0852 . 0 - 4622 / GRO J 0852 - 4642
RX J0852.0-4622 is a supernova remnant discovered in the ROSAT all-sky survey. Spatially coincident 1.157 MeV γ-ray line emission was detected with the COMPTEL instrument on-board of the CGRO. The analysis combining the X-ray and γ-ray data suggests that RX J0852.0-4622 is a close-by and young supernova remnant. Follow-up observations with ASCA show that the two brightest sections of the limb h...
متن کاملTeV gamma-ray Observations of the Supernova Remnant RCW86 with the CANGAROO-II telescope
The supernova remnant RCW86 (G315.4-2.3) has been observed with the CANGAROO-II 10m telescope from Woomera, South Australia. ASCA detected non-thermal X-ray emission from the south-west shell of RCW86, which is brighter than that from SN1006. The multiwavelength spectrum of RCW86 derived from radio and X-ray data indicates that the emission is due to the synchrotron radiation, and it is argued ...
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: The Astrophysical Journal
سال: 2017
ISSN: 1538-4357
DOI: 10.3847/1538-4357/aa6d67