THE INNERMOST COLLIMATION STRUCTURE OF THE M87 JET DOWN TO ∼10 SCHWARZSCHILD RADII

被引:128
作者
Hada, Kazuhiro [1 ,2 ,3 ]
Kino, Motoki [4 ]
Doi, Akihiro [4 ]
Nagai, Hiroshi [2 ]
Honma, Mareki [2 ,3 ]
Hagiwara, Yoshiaki [2 ,3 ]
Giroletti, Marcello [1 ]
Giovannini, Gabriele [1 ,5 ]
Kawaguchi, Noriyuki [2 ,3 ]
机构
[1] INAF Ist Radioastron, I-40129 Bologna, Italy
[2] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
[3] Grad Univ Adv Studies SOKENDAI, Dept Astron Sci, Mitaka, Tokyo 1818588, Japan
[4] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, Sagamihara, Kanagawa 2525210, Japan
[5] Univ Bologna, Dipartimento Fis & Astron, I-40127 Bologna, Italy
基金
日本学术振兴会;
关键词
galaxies: active; galaxies: individual (M87); galaxies: jets; radio continuum: galaxies; ACTIVE GALACTIC NUCLEI; SUPERMASSIVE BLACK-HOLE; HIGH-FREQUENCY VLBI; GAMMA-RAY EMISSION; RELATIVISTIC JETS; MAGNETIC ACCELERATION; ACCRETION DISKS; GALAXY M87; A-ASTERISK; WINDS;
D O I
10.1088/0004-637X/775/1/70
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigated the detailed inner jet structure of M87 using Very Long Baseline Array data at 2, 5, 8.4, 15, 23.8, 43, and 86 GHz, especially focusing on the multi-frequency properties of the radio core at the jet base. First, we measured the size of the core region transverse to the jet axis, defined as W-c, at each frequency nu, and found a relation between W-c and nu: W-c(nu) proportional to nu(-0.71 +/- 0.05). Then, by combining W-c(nu) and the frequency dependence of the core position r(c)(nu), which was obtained in our previous study, we constructed a collimation profile of the innermost jet W-c(r) down to similar to 10 Schwarzschild radii (R-s) from the central black hole. We found that W-c(r) smoothly connects with the width profile of the outer edge-brightened, parabolic jet and then follows a similar radial dependence down to several tens of R-s. Closer to the black hole, the measured radial profile suggests a possible change in the jet collimation shape from the outer parabolic one, where the jet shape tends to become more radially oriented. This result could be related to a magnetic collimation process or/and interactions with surrounding materials at the jet base. The present results shed light on the importance of higher-sensitivity/resolution imaging studies of M87 at 86, 43, and 22 GHz; these studies should be examined more rigorously.
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页数:7
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