Observations of Seyferts by OSSE and parameters of their X-ray/gamma-ray sources
نویسندگان
چکیده
We present a summary of spectra of Seyfert galaxies observed by the OSSE detector aboard Compton Gamma Ray Observatory. We obtain average spectra of Seyferts of type 1 and 2, and find they are well fitted by thermal Comptonization. We present detailed parameter ranges for the plasma temperature and the Compton parameter in the case of spherical and slab geometries. We find both the average and individual OSSE spectra of Seyfert 2s are significantly harder than those of Seyfert 1s, which difference can be due to anisotropy of Compton reflection and/or Thomson-thick absorption. Subject headings: galaxies: active — galaxies: Seyferts — gamma rays: observations
منابع مشابه
Compton Observatory Observations of Agn
The principal results on active galactic nuclei from the Phase 1 observations by the COMPTON Gamma Ray Observatory are presented. These include the detection of a new class of high-energy gamma ray sources by the EGRET instrument and extensive observations of Seyfert galaxies in low-energy gamma rays by OSSE. The identified EGRET sources are associated with core-dominated radio loud objects, OV...
متن کاملX-rays and Soft Gamma-rays from Seyferts, Radio Galaxies, and Black-Hole Binaries
Selected topics dealing with X-ray/soft γ-ray emission from accreting black-hole sources are reviewed. The shape of soft γ-ray spectra of Seyferts observed by OSSE can be well modeled by thermal Comptonization. A very strong correlation between the X-ray slope and the strength of Compton reflection in these sources can then be explained by thermal Comptonization in vicinity of the reflecting co...
متن کاملObservations of Discrete Galactic Sources with Osse
The Oriented Scintillation Spectrometer Experiment (OSSE) on the COMPTON Gamma Ray Observatory has undertaken comprehensive observations of many galactic sources since launch in April 1991. These include investigations of binary X-ray sources, pulsars, several transient X-ray sources observed as Targets-ofOpportunity, and Nova Cygni 1992. Multiple observations of the galactic center region were...
متن کاملX-rays and Gamma-rays from Accretion Flows onto Black Holes in Seyferts and X-ray Binaries
We review observations and theoretical models of Xray/γ-ray spectra of radio-quiet Seyfert galaxies and of Galactic black-hole candidates (in the hard spectral state). The observed spectra share all their basic components: an underlying power law, a Comptonreflection component with an Fe Kα line, low-energy absorption by intervening cold matter, and a highenergy cutoff above ∼ 200 keV. The X-ra...
متن کاملSeyferts and Radio Galaxies
Observations with Compton Gamma Ray Observatory have provided key insights to the high energy emission mechanisms in Active Galactic Nuclei (AGN) and clearly separate them into a class of Blazars, with apparent non-thermal jet emissions often peaking in the EGRET energy band, and into the Seyfert class with emissions more closely related to the accretion disk presumably energizing the nuclear b...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2000