collaborators

9 papers

astro-ph.EP2026

Asymmetric, variable H line profile in planetary mass object SR 12 c

Jun Hashimoto, Yuhiko Aoyama, Michihiro Takami +1

Young, forming planetary-mass objects often exhibit clear signatures of ongoing mass accretion and are thought to accrete material through processes analogous to those operating in…

astro-ph.EP2026

A Hybrid Origin for the Multiple Ring-Gap Structures in the Large Protoplanetary Disk V1094 Sco: A Low-Mass Planet and Secular Gravitational Instability

Masayuki Yamaguchi, Masahiro N. Machida, Ryosuke T. Tominaga +7

High spatial resolution observations reveal that some protoplanetary disks host multiple ring-gap pairs at large stellocentric radii, yet their physical origin remains unsettled. W…

astro-ph.IM2026

GREX-PLUS Science Book v2

PLUS Science Team, Shunsuke Baba, Sirio Belli +52

GREX-PLUS (Galaxy Reionization EXplorer and PLanetary Universe Spectrometer) is a mission candidate for a JAXA strategic L-class mission to be launched in the 2030s. Its primary sc…

astro-ph.SR2026

The Relationship between Accretion and Ionised Ejection among Young Stellar Objects in the Coronet Cluster

Arpan Ghosh, Roberto Galván-Madrid, Johanan Ramírez-Arellano +7

We present results from a coordinated, multi-epoch near-infrared and centimeter radio survey of young stellar objects (YSOs) in the Coronet, aimed at probing the connection between…

astro-ph.SR2025

Morphological and Kinematical Diagnostic of FU Orionis-type Outburst Mechanisms

Jinshi Sai, Eduard I. Vorobyov, Alexandr Skliarevskii +1

We investigated the possibility of determining the mechanism of the FU Orionis-type outburst based on molecular line observations of protoplanetary disks with synthetic observation…

astro-ph.EP2025

Peculiar Disk Substructures Associated with the Young Eruptive Star EX Lupi

Masayuki Yamaguchi, Hauyu Baobab Liu, Michihiro Takami +1

Young eruptive stars such as EXors undergo dramatic accretion outbursts characterized by sudden optical brightenings, yet the underlying physical mechanism remains uncertain. We pr…