Résumé
The multiwavelength observation of the nearby radio galaxy M87 provides a unique opportunity to study in detail processes occurring in active galactic nuclei from radio waves to TeV γ-rays. Here we report the detection of γ-ray emission above 250 GeV from M87 in spring 2007 with the VERITAS atmospheric Cerenkov telescope array and discuss its correlation with the X-ray emission. The γ-ray emission is measured to be pointlike with an intrinsic source radius less than 4.5′. The differential energy spectrum is fitted well by a power-law function: dΦ/dE = (7.4 ± 1.3stat ± 1.5sys)(£/TeV) (-2.31±0.17stat±0.2sys)10-9 m-2 s-1 TeV-1. We show strong evidence for a year-scale correlation between the γ-ray flux reported by TeV experiments and the X-ray emission measured by the ASM RXTE observatory, and discuss the possible short-timescale variability. These results imply that the γ-ray emission from M87 is more likely associated with the core of the galaxy than with other bright X-ray features in the jet.
| langue originale | Anglais |
|---|---|
| Pages (de - à) | 397-403 |
| Nombre de pages | 7 |
| journal | Astrophysical Journal |
| Volume | 679 |
| Numéro de publication | 1 |
| Les DOIs | |
| état | Publié - 20 mai 2008 |
| Modification externe | Oui |
Empreinte digitale
Examiner les sujets de recherche de « Observation of gamma-ray emission from the galaxy M87 above 250 GeV with VERITAS ». Ensemble, ils forment une empreinte digitale unique.Contient cette citation
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver