Studying the Interstellar Medium of H <small class="sc">II</small>/BCD Galaxies Using IFU Spectroscopy

<table> VIMOS-IFU H<svg height="7.9499998" id="M38" style="vertical-align:-0.1638pt" version="1.1" viewbox="0 0 9.7749996 7.9499998" width="9.7749996" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
<g transform="matrix(.017,-0,0,-.017,.062,7.675)"><path d="M545 106q-67 -118 -134 -118q-24 0 -40 37.5t-30 129.5h-2q-47 -72 -103 -119.5t-108 -47.5q-47 0 -76 45.5t-29 119.5q0 113 85 204t174 91q47 0 70 -33.5t43 -119.5h3q32 47 80 140l55 13l10 -9q-47 -80 -138 -201q17 -99 27.5 -136t22.5 -37q23 0 69 61zM333 204
q-14 98 -31 149.5t-50 51.5q-49 0 -94 -70t-45 -164q0 -55 15.5 -86t40.5 -31q70 0 164 150z" id="x1D6FC"></path></g>
</svg> emission line map of the XMP BCD galaxies UM 461 (a) and Tol 65 (b). North is to the top and east to the left. Further details will be presented in a forthcoming paper.</table>

Advances in Astronomy

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Figure 3

Figure 3: Studying the Interstellar Medium of H <small class="sc">II</small>/BCD Galaxies Using IFU Spectroscopy 

Advances in Astronomy

Studying the Interstellar Medium of H II/BCD Galaxies Using IFU Spectroscopy

Figure 3