Research
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2026.07.01
A cosmic lighthouse flashes every 44 minutes in a stellar graveyard
Summary: Astronomers have identified DART J1832-0911, a radio source that flashes every 44.27 minutes from inside the supernova remnant G22.7-0.2. As DART's first astronomical discovery, the source was found with DART and followed up by FAST, which detected a nearly 100% linearly polarized pulse, supporting the idea that the object is most likely a young neutron star slowed by materials left ov...
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2026.06.29
The Blue Eye Pulsar: Breaking Decades of Radio Silence
For decades, one class of neutron stars refused to speak in radio waves.An international research team led by Prof. Di Li of the Department of Astronomy at Tsinghua University has detected radio pulsations from the Central Compact Object (CCO) 1E 1207.4−5209, a young neutron star embedded in the supernova remnant PKS 1209−51/52. Published in Nature Astronomy, the discovery provides some of th...
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2026.06.17
Annual Review Article on the Evolution of Protoplanetary Disks
Recently, Professor Xuening Bai at the Institute for Advanced Study and Department of Astronomy at Tsinghua University published a review article which systematically reviewed the physical mechanisms behind angular momentum transport and long-term evolution of protoplanetary disks, and discussed future prospects on the study of protoplanetary disk gas dynamics and planet formation.Protoplanetar...
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2026.06.08
A Stellar Dynamical Mass Measurement of a Supermassive Black Hole in the Early Universe
Introduction: On June 4, 2026, the journal Science published the paper "A stellar dynamical mass measurement of an inactive black hole at redshift 2," with Meng Gu, an assistant professor in the Department of Astronomy at Tsinghua University, as the 2nd author. Using James Webb Space Telescope (JWST) near-infrared integral field spectroscopy, together with the strong lensing magnification of a ...
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2026.04.14
Deciphering silicate cloud formation in the super-puff planet WASP-107 b
In a recent study led by the Department of Astronomy, Tsinghua University, a group of astronomers explained the silicate cloud features on a super-puff planet WASP-107 b with a self-consistent atmosphere model.The James Webb Space Telescope (JWST) opens up a new window to study the composition of exoplanet atmospheres. Benefiting from its broad wavelength coverage and extraordinary signal-to-no...
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