Detection of 4765 MHz OH Emission in a Preplanetary Nebula: CRL 618-Reference-Cited by-同舟云学术

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Detection of 4765 MHz OH Emission in a Preplanetary Nebula: CRL 618

Published:2019-06-18 Issue:2 Volume:878 Page:90
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Strack A.,Araya E. D.^ORCID,Lebrón M. E.,Minchin R. F.^ORCID,Arce H. G.^ORCID,Ghosh T.^ORCID,Hofner P.,Kurtz S.,Olmi L.^ORCID,Pihlström Y.^ORCID,Salter C. J.

Funder

NSF

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab1f93/pdf

Reference78 articles.

1. The magnetic field of the evolved star W43A

2. A C‐Band Spectral Scan of IRC +10o216

3. QUASI-PERIODIC FORMALDEHYDE MASER FLARES IN THE MASSIVE PROTOSTELLAR OBJECT IRAS 18566+0408

4. FORMALDEHYDE MASERS: EXCLUSIVE TRACERS OF HIGH-MASS STAR FORMATION

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. FAST Detection of OH Emission in the Carbon-rich Planetary Nebula NGC 7027;The Astrophysical Journal;2024-08-28

2. Excited-state OH Masers in the Water Fountain Source IRAS 18460-0151;The Astrophysical Journal Letters;2024-03-20

3. Excited Hydroxyl Outflow in the High-mass Star-forming Region G34.26 + 0.15;The Astrophysical Journal;2023-08-01

4. High-sensitivity observations of molecular lines with the Arecibo Telescope;Monthly Notices of the Royal Astronomical Society;2020-06-26

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