Volume 5 - November 2009
Back Matter
IAU Volume 5 Issue S263 Back Matter
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- Published online by Cambridge University Press:
- 06 April 2010, pp. b1-b9
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Contributed Papers
Some notes on the Inka constellations
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- 29 June 2011, pp. 96-97
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No relation between the vertical velocity component and the absolute magnitude among globular clusters
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- 18 January 2010, pp. 380-383
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Li abundances and chromospheric activity of BY Dra type stars
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- 23 April 2010, pp. 343-344
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A New Approach to the Construction of Dynamical Structure of our Galaxy
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- 21 October 2010, p. 202
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Space clocks to test relativiy: ACES and SAGAS
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- 06 January 2010, pp. 377-389
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Spitzer finds cosmic neon's and sulfur's sweet spot: part III, NGC 6822
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- 09 March 2010, pp. 249-250
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Poster Papers
The star formation histories of fossil group galaxies
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- 13 April 2010, pp. 321-322
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Contributed Papers
Solar cycle changes of large-scale solar wind structure
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- 26 February 2010, pp. 356-358
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What Do Statistics Reveal About the MBH–Mbulge Correlation and Co-Evolution?
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- 03 June 2010, pp. 161-171
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The Effect of the Corotation on the Radial Gradient of Metallicity of Spiral Galaxies
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- 09 March 2010, pp. 251-252
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An iterative method for constructing stellar systems models: how far does it work?
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- 21 October 2010, p. 203
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Connecting Heaven and Man: The role of astronomy in ancient Chinese society and culture
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- 29 June 2011, pp. 98-106
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Rapid solar wind and geomagnetic variability during the ascendant phases of the 11-yr solar cycles
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- 26 February 2010, pp. 359-362
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Poster Papers
A SAURON view of double-barred galaxies
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- 13 April 2010, pp. 323-324
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Contributed Papers
Testing the weak equivalence principle
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- 06 January 2010, pp. 390-401
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Lithium abundances in dwarfs of intermediate age open clusters
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- 23 April 2010, pp. 345-346
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An unusual abundance of T Tauri stars? NIR study of the southern high-mass star-forming region RCW 34
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- 18 January 2010, p. 384
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On the Relation Between Black Hole Mass and Velocity Dispersion in Type 1 and Type 2 AGN
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- 03 June 2010, pp. 172-176
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Open clusters: a program to analyse the color–magnitude diagram with the help of stellar kinematic data
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- 18 January 2010, p. 385
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