A model for the Lin-Shu type density-wave structure of our Galaxy: Line-of-sight and transverse-longitudinal velocities of 242 optically visible open clusters-Reference-Cited by-同舟云学术

A model for the Lin-Shu type density-wave structure of our Galaxy: Line-of-sight and transverse-longitudinal velocities of 242 optically visible open clusters

Published:2015-03 Issue:2 Volume:336 Page:196-207
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr.

Author:

Griv E.,Jiang I.-G.

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/asna.201412139/fullpdf

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4. Galactic kinematics from a sample of young massive stars

5. Giant planet formation by disc instability: flux-limited radiative diffusion and protostellar wobbles

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