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Table 4.

Line-of-sight velocities of D2, D23, D3, and D3.1.

D2 D23 D3 D3.1




Year vHeI [km s−1] vBrγ [km s−1] vHeI [km s−1] vBrγ [km s−1] vHeI [km s−1] vBrγ [km s−1] vHeI [km s−1] vBrγ [km s−1]
2005 −430 −490 −250 −239
2006 −564 −531 −216 −217
2007 −523 −479 −226 −215
2008 −395 −490 −259 −253 −318 −318 145 116
2009 −458 −440
2010 −377 −410 −243 −257 131 138
2011 −401 −387 −281 −266 89 198
2012 −333 −367 −262 −266 160 152
2013 −353 −349 −292 −284 136 145
2014 −346 −368 −335 −332
2015 −294 −319 −324 −325 −660 −710 58 46
2016 −356 −309

Notes. For D2, D23, and D3.1 we can extract these values directly from the spectroscopic analysis of the SINFONI data cubes. The spectroscopic information for D3 in 2008 are extracted from Meyer et al. (2014). We determine an uncertainty of 0.0005 μm. This results in a velocity of ∼36 km s−1 for the HeI and Brγ emission line.

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