DERIVATION OF THE ELECTRON DISTRIBUTION IN SUPERNOVA REMNANT RX J1713.7–3946 VIA A SPECTRAL INVERSION METHOD

نویسندگان
چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Cangaroo-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 کامل

Exploring the Central Compact Object in the RX J0852.0-4622 Supernova Remnant with XMM-Newton

The properties of the presumably young galactic supernova remnant (SNR) RX J0852.0-4622, discovered by ROSAT, are still uncertain. The data concerning the distance to the SNR, its age, and the presence of a compact remnant remain controversial. We report the results of several XMM-Newton observations of CXOU J085201.4-461753, the central compact source in RX J0852.0-4622. The currently prefered...

متن کامل

Gamma-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 کامل

The X–ray Sources at the Center of the Supernova Remnant RX J0852.0−4622

Received ; accepted – 2 – ABSTRACT We present a BeppoSAX observation of the X–ray source AX J0851.9−4617.4 that has been proposed as the neutron star associated to the shell like-supernova remnant RX J0852.0−4622. The image at E>5 keV shows the presence of a new source, SAX J0852.0−4615 , not resolved from AX J0851.9−4617.4 in previous observations. The improved positional accuracy obtained for...

متن کامل

Constraints of age , distance and progenitor of the supernova remnant RX

The discovery of the nearest young supernova remnant RX J0852.0-4622 / GRO J0852-4642 in the Galaxy by ROSAT and COMPTEL has been reported recently. Age and distance are determined to ∼680 years and ∼200 pc by the Xray diameter and the γ-ray line flux of radioactive 44Ti. Here we discuss the implications of the X-ray spectra and of the fact that 1.8 MeV γ-ray line emission from the decay of 26A...

متن کامل

ذخیره 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: 2011

ISSN: 2041-8205,2041-8213

DOI: 10.1088/2041-8205/742/1/l10