Hao-Tse Huang

collaborators

3 papers

astro-ph.HE2026

Evidence of Nuclear Urca Process in the Ocean of Neutron-Star Superburst MAXI J1752 $-$ 457

Hao Huang, Akira Dohi, Amira Aoyama +2

We propose that the rapid cooling of the neutron star following its X-ray superburst in MAXI J1752 $-$ 457 over a period of 4 days, observed by two Japanese satellites, MAXI and Ninj…

astro-ph.GA2024

Gas dynamics in an AGN-host galaxy at $z ≃ 2.6$ : regular rotation, non-circular motions, and mass models

Lingrui Lin, Federico Lelli, Carlos De Breuck +9

The gas dynamics of galaxies provide critical insights into the evolution of both baryons and dark matter (DM) across cosmic time. In this context, galaxies at cosmic noon -- the p…

astro-ph.GA2024

Molecular gas mass measurements of an active, starburst galaxy at $z \approx 2.6$ using ALMA observations of the [CI], CO and dust emission

Hao-Tse Huang, Allison W. S. Man, Federico Lelli +7

We present new ALMA observations of a starburst galaxy at cosmic noon hosting a radio-loud active galactic nucleus: PKS 0529-549 at $z = 2.57$ . To investigate the conditions of its c…

Evidence of Nuclear Urca Process in the Ocean of Neutron-Star Superburst MAXI J1752−457

Gas dynamics in an AGN-host galaxy at z≃2.6: regular rotation, non-circular motions, and mass models

Molecular gas mass measurements of an active, starburst galaxy at z≈2.6 using ALMA observations of the [CI], CO and dust emission

Evidence of Nuclear Urca Process in the Ocean of Neutron-Star Superburst MAXI J1752 $-$ 457

Gas dynamics in an AGN-host galaxy at $z ≃ 2.6$ : regular rotation, non-circular motions, and mass models

Molecular gas mass measurements of an active, starburst galaxy at $z \approx 2.6$ using ALMA observations of the [CI], CO and dust emission