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<p>compared to their star-forming region. For old iPMOs the cold <a href="page.php?w=WISE_J0830%2B2837">WISE J0830+2837</a> shows a V<sub>tan</sub> (tangential <a href="page.php?w=velocity">velocity</a>) of about 100&nbsp;km/s, which is high, but still consistent with formation in our galaxy. For <a href="page.php?w=WISE_1534-1043">WISE 1534-1043</a> one alternative scenario explains this object as an ejected exoplanet due to its high V<sub>tan</sub> of about 200&nbsp;km/s, but its color suggests it is an old metal-poor brown dwarf. Most astronomers</p><p>
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