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

Astron Sci & Technol Res Lab

Guangzhou University

Natl Astron Data Ctr

Jun Yang

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

X. P. Cheng

Korea Astronomy and Space Science Institute

Mai Liao

Universidad Diego Portales

Chinese Academy of Sciences

Xiaoyu Hong

ShanghaiTech University

Chinese Academy of Sciences

Liming Dou

Astron Sci & Technol Res Lab

Guangzhou University

Natl Astron Data Ctr

Tianle Zhao

Natl Astron Data Ctr

Astron Sci & Technol Res Lab

Guangzhou University

Zhongying Fan

Guangzhou University

Natl Astron Data Ctr

Astron Sci & Technol Res Lab

Fupeng Zhang

Guangzhou University

Astron Sci & Technol Res Lab

Natl Astron Data Ctr

Weirong Huang

Guangzhou University

Astron Sci & Technol Res Lab

Natl Astron Data Ctr

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 960 1 1

Ämneskategorier (SSIF 2011)

Astronomi, astrofysik och kosmologi

Atom- och molekylfysik och optik

DOI

10.3847/1538-4357/ad0be6

Mer information

Senast uppdaterat

2026-06-15