Possible Time Correlation between Jet Ejection and Mass Accretion for RW Aur A-Reference-Cited by-同舟云学术

Possible Time Correlation between Jet Ejection and Mass Accretion for RW Aur A

Published:2020-09-17 Issue:1 Volume:901 Page:24
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Takami Michihiro^ORCID,Beck Tracy L.^ORCID,Schneider P. Christian^ORCID,Günther Hans Moritz^ORCID,White Marc^ORCID,Grankin Konstantin,Karr Jennifer L.^ORCID,Ohyama Youichi^ORCID,Coffey Deirdre^ORCID,Liu Hauyu Baobab^ORCID,Galván-Madrid Roberto,Liu Chun-Fan^ORCID,Fukagawa Misato^ORCID,Manset Nadine,Chen Wen-Ping^ORCID,Pyo Tae-Soo^ORCID,Shang Hsien^ORCID,Ray Thomas P.^ORCID,Otsuka Masaaki^ORCID,Chou Mei-Yin^ORCID

Funder

MoST, Taiwan

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abab98/pdf

Reference78 articles.

1. Sub-arcsecond [Fe ii] spectro-imaging of the DG Tauri jet

2. The extreme T Tauri star RW Aur: accretion and outflow variability

3. Astropy: A community Python package for astronomy

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