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<p>(HCN) and <a href="page.php?w=carbon_dioxide">carbon dioxide</a> (CO<sub>2</sub>).</p>

<p>2M1207b shows weak accretion from a disk, inferred from emission lines of <a href="page.php?w=hydrogen">hydrogen</a> and <a href="page.php?w=helium">helium</a> in medium-resolution <a href="page.php?w=NIRSpec">NIRSpec</a> data. Surprisingly 2M1207b does not show absorption due to <a href="page.php?w=methane">methane</a>, which was predicted to be present for this object. It was suggested that very young objects have a L/T-transition starts at a later spectral</p><p>
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