An Enhanced Formation Channel for Galactic Dual-Line Gravitational-Wave Sources: von Zeipel-Lidov-Kozai Effect in Triples Involving Sgr A*

Kavli Affiliate: Lijing Shao | Summary:The dense Galactic Center environment is expected to host compact binary inspirals detectable by future space-borne gravitational wave (GW) observatories (e.g., LISA, TianQin, Taiji) in the millihertz band. Aided by information from these facilities, next-generation ground-based GW detectors (e.g., Cosmic Explorer, Einstein Telescope) can potentially capture gravitational radiation in the […]


Continue.. An Enhanced Formation Channel for Galactic Dual-Line Gravitational-Wave Sources: von Zeipel-Lidov-Kozai Effect in Triples Involving Sgr A*

Mass-Radius Constraints for 2S 0918-549 from an RXTE Superexpansion Burst: A Direct Cooling-Tail Analysis

Kavli Affiliate: Renxin Xu | Summary:Thermonuclear (Type I ) X-ray bursts from accreting neutron stars offer a means to determine neutron-star (NS) mass ($M$) and radius ($R$) and thereby probe the properties of matter at supranuclear density. A subset of these events, photospheric radius-expansion (PRE) bursts, provide a particularly powerful tool to constrain the neutron-star […]


Continue.. Mass-Radius Constraints for 2S 0918-549 from an RXTE Superexpansion Burst: A Direct Cooling-Tail Analysis

Unraveling the mysteries of Jets in peculiar NLSy1 galaxies through multi-wavelength variability

Kavli Affiliate: Luis Ho | Summary:Radio-quiet narrow-line Seyfert 1 galaxies (RQ-NLSy1s) are generally considered to be dominated by thermal emission from the accretion disk. However, recurring 37 GHz radio flares detected from seven RQ-NLSy1s by the Metsahovi Radio Observatory suggest that non-thermal processes may also contribute to their emission. We present a systematic optical and […]


Continue.. Unraveling the mysteries of Jets in peculiar NLSy1 galaxies through multi-wavelength variability

Modeling Tidal Disruption Events and Compact Object Plunges in Nuclear Star Clusters

Kavli Affiliate: Rainer Spurzem | Summary:We study tidal disruption events (TDEs) and compact object inspirals in nuclear star clusters (NSCs) hosting a central supermassive black hole (SMBH), focusing on their role in SMBH growth. Using the STARDISK version of the direct N-body code NBODY6++GPU, we perform pilot simulations with two improved models: one for mass […]


Continue.. Modeling Tidal Disruption Events and Compact Object Plunges in Nuclear Star Clusters

Pulsars and Millisecond Pulsars II: Deep diving into the Evolutionary Mechanisms

Kavli Affiliate: Rainer Spurzem | Summary:This second paper in our series investigates the evolutionary mechanisms that shape pulsars and millisecond pulsars (MSPs) across different astrophysical environments. We focus on the physical processes that govern spin evolution, magnetic field decay, binary interactions, and recycling pathways. Using observational constraints together with theoretical models, we examine how accretion, […]


Continue.. Pulsars and Millisecond Pulsars II: Deep diving into the Evolutionary Mechanisms

Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights

Kavli Affiliate: Rainer Spurzem | Summary:We present a statistical study of pulsars and millisecond pulsars (MSPs) based on multiwavelength observations in the Galactic Field and Globular Clusters. We examine their emission properties, timing behavior, and spatial distributions, and discuss how theoretical models are required to interpret these observational trends. We focus on the magnetic field […]


Continue.. Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights

ALMA 873 $μ$m Polarization Observations of the PDS~70 Disk

Kavli Affiliate: Ruobing Dong | Summary:At a 112.4 pc distance, the PDS70 protoplanetary disk is a rare case that has been confirmed to host two accreting planets. This makes it the most important laboratory for studying dust growth in the context of planet formation. Here we present the first deep, full polarization observations at 873 […]


Continue.. ALMA 873 $μ$m Polarization Observations of the PDS~70 Disk

EPISODE III: The Nested Jet/Outflow Morphology of EC 53 Revealed by JWST and ALMA

Kavli Affiliate: Gregory Herczeg | Summary:We present an extensive study of the structure and kinematics of the jet and outflow of EC 53, a Class I protostar with a quasi-periodic variability, using combined James Webb Space Telescope (JWST) and Atacama Large Millimeter/submillimeter Array (ALMA) observations. ALMA continuum observations resolve a compact disk with a radius […]


Continue.. EPISODE III: The Nested Jet/Outflow Morphology of EC 53 Revealed by JWST and ALMA

A high rate of foreground contaminants toward high-redshift galaxies resolved by JWST

Kavli Affiliate: Linhua Jiang | Summary:We present a study of high-redshift Ly$α$ emitters (LAEs) with multiple components using HST and JWST. High-redshift galaxies are mostly point-like objects on ground-based images, but they often exhibit multiple components in higher spatial resolution images. JWST for the first time allow detailed analyses on these individual components. We collect […]


Continue.. A high rate of foreground contaminants toward high-redshift galaxies resolved by JWST

Modeling the Dynamics and Thermochemistry for the Outer Atmospheres of the Ultra-hot Jupiter WASP-121b

Kavli Affiliate: Lile Wang |Summary:We present three-dimensional simulations of the ultra-hot Jupiter (UHJ) WASP-121b from the planetary surface to extended outflows, coupling hydrodynamics with consistent non-equilibrium thermochemistry, ray-tracing radiative transfer, and hydrodynamics using the GPU-accelerated Kratos framework. The fiducial model exhibits several atmospheric layers, including the lower atmospheres controlled by day-night circulation, and transonic photoevaporative […]


Continue.. Modeling the Dynamics and Thermochemistry for the Outer Atmospheres of the Ultra-hot Jupiter WASP-121b