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    <lastmod>2024-10-01</lastmod>
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      <image:caption>Spatial anticorrelation between H13CO+ and H218O in the protostellar envelope around NGC1333 IRAS2A observed with NOEMA. Figure from van ‘t Hoff et al. (2018a).</image:caption>
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      <image:caption>Illustration of the effect of disk temperature on the composition of the planet-forming material upon crossing different sublimation fronts. © Merel van ‘t Hoff</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/5ba215cb2714e57120063f57/70aa3473-0cfc-4fb6-9bd4-d527fe9a0f6d/TemperatureOverview.png</image:loc>
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      <image:caption>Overview of midplane temperature profiles in young (Class 0 and I) disks and mature (Class II) disks. Figure from van ‘t Hoff et al. (2019, PhD thesis). The temperature profile for IRAS 16293A is from van ‘t Hoff et al. (2020a), IRAS 04302 is from van ‘t Hoff et al. (2020c), L1527 is from van ‘t Hoff et al. (2018b), and TW Hya is from Schwarz et al. (2016).</image:caption>
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      <image:caption>Schematic overview of low-mass star formation. © Merel van ‘t Hoff</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/5ba215cb2714e57120063f57/1544530318558-550IHDDI571CJAS35QTZ/V883Ori_spectrum.png</image:loc>
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      <image:caption>ALMA spectrum of the disk around the outbursting protostar V883 Ori obtained with only 1 minute of integration. Figure from van ‘t Hoff et al. (2018c).</image:caption>
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    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/5ba215cb2714e57120063f57/0acc4399-a56e-47e3-8cda-39a047fc0489/Cartoon_CarbonGrainDestruction.png</image:loc>
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      <image:caption>Schematic of the inner region around a protostar and the predicted chemical effects of the destruction of carbonaceous grains inside the soot line. Figure adapted from van ‘t Hoff et al. (2020b).</image:caption>
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      <image:caption>ALMA observations of a young disk. © Merel van ‘t Hoff</image:caption>
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