Statistical analysis of the flux of micrometeoroids at Mercury from both cometary and asteroidal components (Corrigendum)
1 INAF-Astronomical Observatory of Padova, Vicolo dell’Osservatorio 5, 35131 Padova, Italy
e-mail: patrizia.borin@oapd.inaf.it; gabriele.cremonese@oapd.inaf.it
2 Department of Physics and Astronomy, University of Padova, via Marzolo 8, 35131 Padova, Italy
e-mail: marzari@pd.infn.it
Key words: methods: statistical / meteorites, meteors, meteoroids / comets: general / planets and satellites: individual: Mercury / errata, addenda
Figure 4 of the original manuscript shows the velocity distribution curves at Mercury for both asteroidal and cometary sources of dust. The curves and the values in the axis are correct, but the labels are wrong. The right labels are: the velocity of dust particles v on the x-axis and the velocity distribution function f(v) on the y-axis.
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Fig. 4 Velocity distribution of asteroidal and cometary dust particles at Mercury. |
| Open with DEXTER | |
© ESO, 2016
All Figures
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Fig. 4 Velocity distribution of asteroidal and cometary dust particles at Mercury. |
| Open with DEXTER | |
| In the text | |