The nearby spiral density‐wave structure of the Galaxy: Line‐of‐sight and longitudinal velocities of 61 masers-Reference-Cited by-同舟云学术

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The nearby spiral density‐wave structure of the Galaxy: Line‐of‐sight and longitudinal velocities of 61 masers

Published:2017-07 Issue:6 Volume:338 Page:729-739
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron.Nachr./AN

Author:

Griv E.¹,Jiang I.‐G.²,Hou L.‐G.³,Ngeow C.‐C.⁴

Affiliation:

1. Department of Physics Ben‐Gurion University of the Negev Beer‐Sheva Israel

2. Department of Physics National Tsing‐Hua University Hsin‐Chu Taiwan

3. National Astronomical Observatories Chinese Academy of Sciences Beijing China

4. Graduate Institute of Astronomy National Central University Jhong‐Li Taiwan

Funder

Israel Science Foundation

National Natural Science Foundation of China

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.201713150

Reference95 articles.

1. DYNAMICS OF NON-STEADY SPIRAL ARMS IN DISK GALAXIES

2. Modal approach to the morphology of spiral galaxies. I - Basic structure and astrophysical viability.

3. On the kinematics of O and B stars

4. Tracing the Galactic spiral structure with embedded clusters

Cited by 3 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. The nearby spiral density-wave structure of the Galaxy: line-of-sight velocities of the Gaia DR2 OB stars;Monthly Notices of the Royal Astronomical Society;2021-02-23

2. Precise radio astrometry and new developments for the next generation of instruments;The Astronomy and Astrophysics Review;2020-09-29

3. The Lin–Shu type density–wave structure of the Galaxy: Line-of-sight velocities of selected 37354 RAVE DR5 stars;New Astronomy;2019-01

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