High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22
Jinghua Yuan
(1)
,
Jin-Zeng Li
(1)
,
Yuefang Wu
(2)
,
Simon Ellingsen
(3)
,
Christian Henkel
(4)
,
Ke Wang
(5)
,
Tie Li
(6)
,
Hong-Li Li
(7)
,
Annie Zavagno
(8)
,
Zhiyuan Ren
(1)
,
Ya-Fang Huang
(1)
1
CAS -
Chinese Academy of Sciences [Beijing]
2 Peking University [Beijing]
3 UTAS - University of Tasmania [Hobart, Australia]
4 MPIFR - Max-Planck-Institut für Radioastronomie
5 ESO - European Southern Observatory
6 KASI - Korea Astronomy and Space Science Institute
7 CUHK - The Chinese University of Hong Kong [Hong Kong]
8 LAM - Laboratoire d'Astrophysique de Marseille
2 Peking University [Beijing]
3 UTAS - University of Tasmania [Hobart, Australia]
4 MPIFR - Max-Planck-Institut für Radioastronomie
5 ESO - European Southern Observatory
6 KASI - Korea Astronomy and Space Science Institute
7 CUHK - The Chinese University of Hong Kong [Hong Kong]
8 LAM - Laboratoire d'Astrophysique de Marseille
Ke Wang
- Fonction : Auteur
- PersonId : 763205
- ORCID : 0000-0002-5776-0815
Annie Zavagno
- Fonction : Auteur
- PersonId : 175663
- IdHAL : annie-zavagno
- ORCID : 0000-0001-9509-7316