A Centiparsec-scale Compact Radio Core in the Nearby Galaxy M60
Artikel i vetenskaplig tidskrift, 2024
M60, an elliptical galaxy located 16.5 Mpc away, has an active nucleus with a very low luminosity and an extremely low accretion rate. Its central supermassive black hole (SMBH) has a mass of M BH ∼ 4.5 × 109 M ⊙ and a Schwarzschild radius corresponding to R S ∼ 5.4 μas. To investigate the nature of its innermost radio nucleus, data from the Very Long Baseline Array (VLBA) at 4.4 and 7.6 GHz were reduced. The VLBA images reveal a compact component with total flux densities of ∼20 mJy at both frequencies, a size of ≤0.27 mas (99.7% confidence level), about 0.022 pc (50 R S) at 7.6 GHz, and a brightness temperature of ≥6 × 109 K. This suggests that the observed centiparsec-scale compact core could be attributed to a nonthermal jet base or an advection-dominated accretion flow (ADAF) with nonthermal electrons. The extremely compact structure also supports the presence of an SMBH in the center. Our results indicate that M60 is a promising target for broadband very long baseline interferometry observations at millimeter wavelengths to probe ADAF scenarios and tightly constrain the potential photon ring (about 28 μas) around its SMBH.
Författare
X. F. Li
National Astronomical Data Center
Guangzhou University
Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province
Jun Yang
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
X. P. Cheng
Korea Astronomy and Space Science Institute
Mai Liao
Chinese Academy of Sciences
Universidad Diego Portales
Xiaoyu Hong
Shanghai Astronomical Observatory
Chinese Academy of Sciences
ShanghaiTech University
Liming Dou
Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province
National Astronomical Data Center
Guangzhou University
Tianle Zhao
Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province
National Astronomical Data Center
Guangzhou University
Zhongying Fan
National Astronomical Data Center
Guangzhou University
Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province
Fupeng Zhang
Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province
National Astronomical Data Center
Guangzhou University
Weirong Huang
Guangzhou University
Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province
National Astronomical Data Center
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 960 1 1Ämneskategorier
Astronomi, astrofysik och kosmologi
Atom- och molekylfysik och optik
DOI
10.3847/1538-4357/ad0be6