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Home All issues A&A, 473 1 (2007) 31-40 Article references

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Cited article:

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

E. Griv, I.‐G. Jiang, L.‐G. Hou and C.‐C. Ngeow
Astronomische Nachrichten 338 (6) 729 (2017)
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Impact of cosmological satellites on the vertical heating of the Milky Way disc

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Spectrum of Lin–Shu-type density waves in the Galaxy: a number of discrete spiral modes of collective oscillations?

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

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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

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Astronomische Nachrichten 336 (2) 196 (2015)
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Dissecting simulated disc galaxies – II. The age–velocity relation

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Numerical code for multi-component galaxies: fromN-body to chemistry and magnetic fields

S A Khoperskov, E O Vasiliev, A V Khoperskov and V N Lubimov
Journal of Physics: Conference Series 510 012011 (2014)
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A simple and accurate approximation for the Q stability parameter in multicomponent and realistically thick discs

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Global gravitationally organized spiral waves and the structure of NGC 5247

S. A. Khoperskov, A. V. Khoperskov, I. S. Khrykin, et al.
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Numerical modelling of the vertical structure and dark halo parameters in disc galaxies

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High resolution in z ‐direction: The simulation of disc‐bulge‐halo galaxies using the particle‐mesh code SUPERBOX

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Unstable Disk Galaxies. II. The Origin of Growing and Stationary Modes

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The Astrophysical Journal 689 (1) 134 (2008)
https://doi.org/10.1086/592556