[N i] 10400/10410 Å Lines as Possible Disk Wind Tracers in a Young Intermediate-mass Star

In this study, we performed high-resolution near-infrared (NIR) spectroscopy ( R = 28,000; λ = 0.90–1.35 μ m) with a high signal-to-noise ratio on HD 200775, a very young (∼0.1 Myr old) and massive intermediate-mass star (a binary star with a mass of about 10 M _⊙ each) with a protoplanetary disk. T...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Haruki Katoh, Chikako Yasui, Yuji Ikeda, Naoto Kobayashi, Noriyuki Matsunaga, Sohei Kondo, Hiroaki Sameshima, Satoshi Hamano, Misaki Mizumoto, Hideyo Kawakita, Kei Fukue, Shogo Otsubo, Keiichi Takenaka
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Protoplanetary disks Stellar winds Star formation Herbig Ae/Be stars T Tauri stars Pre-main sequence stars
Online Access:	https://doi.org/10.3847/1538-4357/ad2842