Is this you? As a journalist, you can create a free Muck Rack account to customize your profile, list your contact preferences, and upload a portfolio of your best work.
Claim your profile
Abstract: The nearby radio galaxy M87 is a prime target for studying black hole accretion and jet formation1,2. Event Horizon Telescope observations of M87 in 2017, at a wavelength of 1.3 mm, revealed a ring-like structure, which was interpreted as gravitationally lensed emission around a central black hole3. Here we report images of M87 obtained in 2018, at a wavelength of 3.5 mm, showing that the compact radio core is spatially resolved.
Bui Chung1, LI YIN (JESSICA) LIN2, Chun Ji Lin1, Hung Yi Chiou3* and Ya Wen Chiu4 1Taipei Medical University, Taiwan 2National Taipei University of Nursing and Health Sciences, Taiwan 3Institute of Population Health Sciences, National Health Research Institutes (Taiwan), Taiwan 4Kaohsiung Medical University, Taiwan Provisionally accepted: The final, formatted version of the article will be published soon.
As a journalist, you can create a free Muck Rack account to customize your profile, list your contact preferences, and upload a portfolio of your best work.
