Vertical gradients of azimuthal velocity in a global thin-disc model of spiral galaxies NGC 2403, NGC 4559, NGC 4302 and NGC 5775

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Monthly Notices of the Royal Astronomical Society, Vol. 412, Iss. 1, 2011-03 ,pp. : 331-336

Oxford University Press

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Towards a fully consistent Milky Way disc model – II. The local disc model and SDSS data of the NGP region

By Just A.   Gao S.   Vidrih S.  

Monthly Notices of the Royal Astronomical Society, Vol. 411, Iss. 4, 2011-03 ,pp. : 2586-2595

Oxford University Press

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Towards a fully consistent Milky Way disc model – I. The local model based on kinematic and photometric data

By Just A.   Jahreiß H.  

Monthly Notices of the Royal Astronomical Society, Vol. 402, Iss. 1, 2010-02 ,pp. : 461-478

Oxford University Press

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Abundance Gradients as a tool for understanding the Formation of the Milky Way

By Chiappini Cristina  

Astrophysics and Space Science, Vol. 281, Iss. 1-2, 2002-07 ,pp. : 253-256

Springer Publishing Company

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Two groups within the thick disc of the Milky Way?

By Stanford Laura M.   Lambert David L.  

Monthly Notices of the Royal Astronomical Society, Vol. 424, Iss. 3, 2012-08 ,pp. : 2118-2129

Oxford University Press

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