Evolution of the outflow traced by water masers in the evolved star IRAS 18043 - 2116
Paper i proceeding, 2022

We present the spectral and spatial evolution of H2O masers associated with IRAS 18043-2116, a well-known water fountain hosting a high-velocity collimated jet, which has been found in the observations with the 45 m telescope of Nobeyama Radio Observatory and the Australia Telescope Compact Array. We found new highest velocity components of the H2O masers, with which the resulting velocity spread of ≃ 540 km s-1 breaks the speed record of fast jets/outflows in this type of sources.

stars: individuals (IRAS 18043-2116)

stars: AGB and post-AGB

masers

Författare

L. Uscanga

Universidad de Guanajuato

H. Imai

Kagoshima University

J. F. Gomez

Instituto de Astrofisica de Andalucía (IAA)

Daniel Tafoya

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

G. Orosz

JOINT INSTITUTE FOR V.L.B.I. IN EUROPE (J.I.V.E.)

T. P. McCarthy

University of Tasmania

Yuhki Hamae

Kagoshima University

Kei Amada

Kagoshima University

Proceedings of the International Astronomical Union

1743-9213 (ISSN) 1743-9221 (eISSN)

Vol. 18 338-342

Ämneskategorier

Astronomi, astrofysik och kosmologi

Oceanografi, hydrologi, vattenresurser

DOI

10.1017/S1743921323002156

Mer information

Senast uppdaterat

2024-03-12