activity
20242026
collaborators

10 papers

astro-ph.HE2026

The Distinctive Evolution and Spectral Energy Distribution of Binary Massive Black Hole Accretion

Yue Xu, Fu-Guo Xie, Ya-Ping Li +2

Binary (super-)massive black holes (BHs) are expected to reside in the center of some galaxies. In this work, we re-visit accretion onto binary massive BHs, incorporating recent ad…

astro-ph.HE2026

A 0.03 Hz Radio Quasi-periodic Oscillation During the 2025 Flare of GRS 1915+105

Ya Xing Li, Lei Liu, Wu Jiang +3

Our weekly-cadence radio monitoring campaign captured a bright flare in 2025 from the microquasar GRS 1915+105, observed simultaneously in the S- and X-bands (2.25 GHz and 8.42 GHz…

astro-ph.SR2026

TESS observations of the Pleiades cluster: a nursery for delta Scuti stars

Timothy R. Bedding, Simon J. Murphy, Courtney Crawford +8

We studied 89 A- and F-type members of the Pleiades open cluster, including five escaped members. We measured projected rotational velocities (v sin i) for 49 stars and confirmed t…

astro-ph.EP2026

Planet Migration in Protoplanetary Disks with Rims

Zhuoya Cao, Ya-Ping Li, Douglas N. C. Lin +1

Complex structures, including sharp edges, rings and gaps, have been commonly observed in protoplanetary disks with or without planetary candidates. Here we consider the possibilit…

astro-ph.EP2025

Outward Migration of a Gas Accreting Planet: A Semi-Analytical Formula

Shigeru Ida, Ya-Ping Li, Jun-Peng Pan +2

Type II orbital migration is a key process to regulate the mass and semimajor axis distribution of exoplanetary giant planets. The conventional formula of type II migration general…

astro-ph.EP2025

Concurrent Accretion and Migration of Giant Planets in their Natal Disks with Consistent Accretion Torque (II): Parameter Survey and Condition for Outward Migration

JunPeng Pan, Ya-Ping Li, Yi-Xian Chen +2

Migration typically occurs during the formation of planets and is closely linked to the planetary formation process. In classical theories of non-accreting planetary migration, bot…