Harada, Naoto http://orcid.org/0000-0002-8217-7509
Tokuda, Kazuki http://orcid.org/0000-0002-2062-1600
Yamasaki, Hayao
Sato, Asako http://orcid.org/0000-0001-5817-6250
Omura, Mitsuki http://orcid.org/0000-0002-7951-1641
Hirano, Shingo http://orcid.org/0000-0002-4317-767X
Onishi, Toshikazu http://orcid.org/0000-0001-7826-3837
Tachihara, Kengo http://orcid.org/0000-0002-1411-5410
Machida, Masahiro N. http://orcid.org/0000-0002-0963-0872
Funding for this research was provided by:
National Astronomical Observatory of Japan (2022-22B)
MEXT ∣ Japan Society for the Promotion of Science (JP17H06360)
MEXT ∣ Japan Society for the Promotion of Science (JP17K05387)
MEXT ∣ Japan Society for the Promotion of Science (JP17KK0096)
MEXT ∣ Japan Society for the Promotion of Science (JP21K13962)
MEXT ∣ Japan Society for the Promotion of Science (JP21H00049)
MEXT ∣ Japan Society for the Promotion of Science (JP21K03617)
MEXT ∣ Japan Society for the Promotion of Science (JP21H00046)
Article Title: Crescent-shaped Molecular Outflow from the Intermediate-mass Protostar DK Cha Revealed by ALMA
Journal Title: The Astrophysical Journal
Article Type: paper
Copyright Information: © 2023. The Author(s). Published by the American Astronomical Society.
Publication dates
Date Received: 2022-11-29
Date Accepted: 2023-02-02
Online publication date: 2023-03-07