Is the core of M87 the source of its TeV emission? Implications for unified schemes

被引:57
作者
Georganopoulos, M
Perlman, ES
Kazanas, D
机构
[1] Univ Maryland Baltimore Cty, Dept Phys, Joint Ctr Astrophys, Baltimore, MD 21250 USA
[2] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA
关键词
galaxies : active; quasars : general; quasars : individual (M87); radiation mechanisms : nonthermal; X-rays : galaxies;
D O I
10.1086/498714
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
M87 has recently been shown to be a TeV source that is likely to be variable. Based on this and on contemporaneous optical and X-ray monitoring, we argue that the source of the TeV emission is the core of M87 and not one of two jet knots ( HST-1 and A), with an X-ray brightness comparable to that of the core. We model the TeV emission in the core as inverse Compton (IC) emission from the base of the jet. Homogeneous models fail to reproduce the spectral energy distribution ( SED) and, in particular, the TeV flux. They also fail to comply with the unified scheme of BL Lacertae (BL) objects and FR I radio galaxies. A jet that decelerates from a Lorentz factor Gamma similar to 20 down to Gamma similar to 5 over a length of similar to 0.1 pc reproduces the observed SED of the M87 core and, when aligned with the line of sight, produces a SED similar to those of TeV BLs. The TeV flux in the decelerating jet model is successfully reproduced as upstream Compton (UC) scattering, a recently identified emission mechanism, in which energetic electrons of the upstream faster flow upscatter the low-energy photons produced in the slower downstream part of the flow.
引用
收藏
页码:L33 / L36
页数:4
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