Inner Warm Disk of ESO Hα279a Revealed by NA i and CO Overtone Emission Lines-Reference-Cited by-同舟云学术

Inner Warm Disk of ESO Hα279a Revealed by NA i and CO Overtone Emission Lines

Published:2017-07-17 Issue:1 Volume:844 Page:4
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Lyo A-Ran,Kim Jongsoo,Lee Jae-Joon^ORCID,Kim Kyoung-Hee^ORCID,Kang Jihyun,Byun Do-Young^ORCID,Mace Gregory,Sokal Kimberly R.,Park Chan,Chun Moo-Young,Oh Heeyoung,Yu Young Sam,Oh Jae Sok,Jeong Ueejeong,Kim Hwihyun,Pak Soojong,Hwang Narae,Park Byeong-Gon,Lee Sungho,Kaplan Kyle,Lee Hye-In,Le Huynh Anh Nguyen,Jaffe Daniel,

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/844/i=1/a=4/pdf

Reference62 articles.

1. High Spectral Resolution Near-IR Observations of ESO-Hα 279A and 279B

2. Detections of Rovibrational H2Emission from the Disks of T Tauri Stars

3. Quiescent H2Emission From Pre‐Main‐Sequence Stars in Chamaeleon I

4. Evidence for an inner molecular disk around massive Young Stellar Objects

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