Chapter 2 Galactic Gamma-ray Sources *

نویسندگان

چکیده

Abstract In the ? -ray sky, highest fluxes come from Galactic sources: supernova remnants (SNRs), pulsars and pulsar wind nebulae, star forming regions, binaries micro-quasars, giant molecular clouds, center, large extended area around plane. The radiation mechanisms of emission physics emitting particles, such as origin, acceleration, propagation, are very high astrophysical significance. A variety theoretical models have been suggested for relevant physics, with energies E ?10 14 eV expected to be crucial in testing them. particular, this energy band is a direct window test at which maximum particle can accelerated sources whether most probable source candidates center SNRs “PeVatrons”. Designed aiming (VHE, >100 GeV) observation, LHAASO will powerful instrument these studies. Over past decade, great advances made VHE astronomy. More than 170 observed, among them, 42 fall field-of-view. With sensitivity 10 milli-Crab, not only provide accurate spectra known sources, but also search new TeV-PeV sources. following sub-sections, observation all discussed details.

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

Observations of Galactic Gamma-ray Sources

The High Energy Stereoscopic System (H.E.S.S.) is a system of four imaging atmospheric Cherenkov telescopes which commenced full operation in the Khomas Highland of Namibia in December 2003 , at an altitude of 1800 m. The experiment is run by an international collaboration of mostly European institutes. It is built for very-high-energy (VHE) gamma-ray astronomy, exploiting the energy range abov...

متن کامل

The GeV-TeV Connection in galactic gamma-ray sources

Recent observations by atmospheric Cherenkov telescopes such as H.E.S.S. and MAGIC have revealed a large number of new sources of very-high-energy (VHE) gamma-rays above 100 GeV, mostly concentrated along the Galactic plane. At lower energies (100 MeV – 10 GeV) the satellite-based instrument EGRET revealed a population of sources clustering along the Galactic Plane. Given their adjacent energy ...

متن کامل

Variable Unidentified Gamma-ray Sources near the Galactic Plane

In a recent paper, Romero et al. (1999) have presented the results of a positional correlation analysis of the low-latitude unidentified gamma-ray sources in the Third EGRET catalog with complete lists of galactic objects like supernova remnants, early type stars with strong stellar winds, and OB associations (considered as pulsar tracers). We have now carried out a study of those 42 sources at...

متن کامل

Blazars, Gamma Ray Bursts and Galactic superluminal sources

BeppoSAX is best known for its role in the disclosure of the Gamma–Ray Burst mystery, but it has also improved our understanding of jetted sources in general, and blazars in particular. On the interpretational side, we are curious to see if all sources with relativistic jets (or “flying pancakes”, as in GRBs) are controlled by the same basic physics, despite the very different lifetimes and beh...

متن کامل

Observation of Galactic Gamma-ray Sources with VERITAS

We report on VERITAS observations at energies above 200 GeV of known or potential galactic γ-ray sources. The observed objects comprise pulsars, pulsar wind nebulae, high-mass X-ray binaries and gamma-ray sources with unknown counterparts in other wavelengths. Among the highlights are the observation of variable gamma-ray emission from the X-ray binary LS I +61 303 and the detection of MGRO J19...

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: Chinese Physics C

سال: 2022

ISSN: ['1674-1137', '2058-6132']

DOI: https://doi.org/10.1088/1674-1137/ac3fa8