activity
20142026
most citedThe ALMA Survey of 70 m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

207 citations · 893 across the 40 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

Protoplanetary Disk Evolution in a Low-Metallicity Environment: JWST's First Mid-Infrared Census of Low-Mass Stars

Chikako Yasui, Natsuko Izumi, Masao Saito +3

This study presents the first high-resolution, high-sensitivity mid-infrared (MIR) investigation of protoplanetary disks in a low-metallicity environment, using JWST/NIRCam and MIR…

astro-ph.SR2022★ 8 cited

A Very Metal-poor RR Lyrae Star with a Disk Orbit Found in the Solar Neighborhood

Noriyuki Matsunaga, Akinori Itane, Kohei Hattori +28

Metal-deficient stars are important tracers for understanding the early formation of the Galaxy. Recent large-scale surveys with both photometric and spectroscopic data have report…

astro-ph.SR2019★ 6 cited

Possible progression of mass flow processes around young intermediate-mass stars based on high-resolution near-infrared spectroscopy. I. Taurus

Chikako Yasui, Satoshi Hamano, Kei Fukue +12

We used the WINERED spectrograph to perform near-infrared high-resolution spectroscopy (resolving power ,000) of 13 young intermediate-mass stars in the Taurus star-forming…

astro-ph.SR2019★ 23 cited

FeI lines in 0.91-1.33 m spectra of red giants for measuring the microturbulence and metallicities

Sohei Kondo, Kei Fukue, Noriyuki Matsunaga +16

For a detailed analysis of stellar chemical abundances, high-resolution spectra in the optical have mainly been used, while the development of near-infrared (NIR) spectrograph has…

astro-ph.SR2018★ 2 cited

WINERED high-resolution near-infrared line catalog: A-type star

H. Sameshima, Y. Ikeda, N. Matsunaga +13

We present a catalog of absorption lines in the z', Y, and J bands that we identified in 21 Lyn, a slowly rotating A0.5 V star. We detected 155 absorption features in the high-reso…

astro-ph.SR2018★ 5 cited

A newly-identified emission-line region around P Cygni

Misaki Mizumoto, Naoto Kobayashi, Satoshi Hamano +12

We present a high-resolution () near-infrared (9,100-13,500 ) long-slit spectrum of P Cygni obtained with the newly commissioned WINERED spectrograph in Japan.…

astro-ph.SR2016

Herbig Ae/Be candidate stars in the innermost Galactic disk: Quartet cluster

Chikako Yasui, Naoto Kobayashi, Satoshi Hamano +4

In order to investigate the Galactic-scale environmental effects on the evolution of protoplanetary disks, we explored the near-infrared (NIR) disk fraction of the Quartet cluster,…

astro-ph.SR2015★ 24 cited

Low-metallicity Young Clusters in the Outer Galaxy I. Sh 2-207

Chikako Yasui, Naoto Kobayashi, Alan T. Tokunaga +2

To study star formation in low metallicity environments ([M/H] ~ -1 ,dex), we obtained deep near-infrared (NIR) images of Sh 2-207 (S207), which is an HII region in the outer Galax…