Trigonometric parallax and proper motion of Sagittarius A* measured by VERA using the new broad-band back-end system OCTAVE-DAS
| Autor: | Oyama, Tomoaki, Nagayama, Takumi, Yamauchi, Aya, Sakai, Daisuke, Imai, Hiroshi, Honma, Mareki, Asakura, Yu, Hada, Kazuhiro, Hagiwara, Yoshiaki, Hirota, Tomoya, Jike, Takaaki, Kono, Yusuke, Suzuki, Syunsaku, Kobayashi, Hideyuki, Kawaguchi, Noriyuki |
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| Rok vydání: | 2024 |
| Předmět: | |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1093/pasj/psad088 |
| Popis: | We successfully measured the trigonometric parallax of Sagittarius A* (Sgr A*) to be $117\pm17$ micro-arcseconds ($\mu$as) using the VLBI Exploration of Radio Astrometry (VERA) with the newly developed broad-band signal-processing system named OCTAVE-DAS. The measured parallax corresponds to a Galactocentric distance at the Sun of $R_0 = 8.5^{+1.5}_{-1.1}$ kpc. By combining the astrometric results with VERA and the Very Long Baseline Array (VLBA) over a monitoring period of 25 years, the proper motion of Sgr A* is obtained to be $(\mu_\alpha, \mu_\delta) = (-3.133\pm0.003, -5.575\pm0.005)$ mas yr$^{-1}$ in equatorial coordinates, corresponding to $(\mu_l, \mu_b) = (-6.391\pm0.005, -0.230\pm0.004)$ mas yr$^{-1}$ in Galactic coordinates. This gives an angular orbital velocity of the Sun of $\Omega_\odot = 30.30 \pm 0.02$ km s$^{-1}$ kpc$^{-1}$. We find upper limits to the core wander, $\Delta \theta < 0.20$ mas (1.6 AU), peculiar motion, $\Delta \mu < 0.10$ mas yr$^{-1}$ (3.7 km s$^{-1}$), and acceleration, $a < 2.6$ $\mu$as yr$^{-2}$ (0.10 km s$^{-1}$ yr$^{-1}$) for Sgr A*. Thus, we obtained upper mass limits of $\approx$ 3 $\times$ 10$^{4}$$M_{\odot}$ and $\approx$ 3 $\times$ 10$^{3}$$M_{\odot}$ for the supposed intermediate-mass black holes at 0.1 and 0.01 pc from the Galactic center, respectively. Comment: 15 pages, 9 figures, accepted for publication in the Publications of the Astronomical Society of Japan |
| Databáze: | arXiv |
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