26Al imaging details from COMPTEL

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود 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

Image reconstruction of COMPTEL 1.8 MeV 26Al line data

We present a new algorithm, called Multiresolution Regularized Expectation Maximization (MREM), for the reconstruction of γ-ray intensity maps from COMPTEL data. The algorithm is based on the iterative Richardson-Lucy scheme to which we added a wavelet thresholding step in order to eliminate image-noise in the reconstruction. The wavelet thresholding explicitly accounts for spatial correlations...

متن کامل

A multiwavelength comparison of COMPTEL 1.8 MeV 26Al line data

We search for correlations between 1.809 MeV γ-ray line emission, attributed to the radioactive decay of 26Al, and intensity distributions observed at other wavelengths by confronting CGRO COMPTEL 1.8 MeV data with an extended database of all-sky maps. The database contains 31 all-sky maps, covering the entire explored wavelength range from the radio band up to high-energy gamma-rays. Different...

متن کامل

COMPTEL ALL-SKY IMAGING AT 2.2 MeV

It is now generally accepted that accretion of matter onto a compact object (white dwarf, neutron star or black hole) is one of the most efficient processes in the universe for producing high energy radiations. The efficient conversion of gravitational potential enegy into kinetic energy is believed to be the primary source of power for X-ray binaries and for Active Galactic Nuclei (AGN). An un...

متن کامل

Maximum Entropy Imaging of Comptel Data

The Maximum Entropy method is a practical technique for generating intensity skymaps from Compton-telescope data. The application of the method to COMPTEL data for point sources and large-scale emission is described. New developments in the method are illustrated.

متن کامل

Radioactive 26Al from the Scorpius-Centaurus association

Context. The Scorpius-Centaurus association is the most-nearby group of massive and young stars. As nuclear-fusion products are ejected by massive stars and supernovae into the surrounding interstellar medium, the search for characteristic γ-rays from radioactivity is one way to probe the history of activity of such nearby massive stars on a My time scale through their nucleosynthesis. 26Al dec...

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: Advances in Space Research

سال: 1995

ISSN: 0273-1177

DOI: 10.1016/0273-1177(94)00050-b