Mathematical Research Data Initiative
Main page
Recent changes
Random page
Help about MediaWiki
Create a new Item
Create a new Property
Create a new EntitySchema
Merge two items
In other projects
Discussion
View source
View history
Purge
English
Log in

The Lin-Shu type density wave structure of our galaxy: line-of-sight velocities of 396 HII regions

From MaRDI portal
Publication:748301
Jump to:navigation, search

DOI10.1007/s10569-015-9638-zzbMath1429.85005OpenAlexW1457167903MaRDI QIDQ748301

D. Kharzeev

Publication date: 20 October 2015

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10569-015-9638-z


zbMATH Keywords

spiral structuregalaxycygnus-orion spiral armgalaxy kinematics


Mathematics Subject Classification ID

Galactic and stellar structure (85A15)




Cites Work

  • Unnamed Item
  • Unnamed Item
  • Optimizing insurance and reinsurance in the dynamic Cramér-Lundberg model
  • Multifractal diffusion in NASDAQ
  • Fine-scale density wave structure of Saturn's rings: A hydrodynamic theory


This page was built for publication: The Lin-Shu type density wave structure of our galaxy: line-of-sight velocities of 396 HII regions

Retrieved from "https://portal.mardi4nfdi.de/w/index.php?title=Publication:748301&oldid=12663886"
Tools
What links here
Related changes
Special pages
Printable version
Permanent link
Page information
MaRDI portal item
This page was last edited on 30 January 2024, at 11:24.
Privacy policy
About MaRDI portal
Disclaimers
Imprint
Powered by MediaWiki