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Bradford, M. Galametz, M. Griffin, M. J. Page, M. Pohlen, M. R. P. Schirm, M. Sauvage, M. Symeonidis, M. Trichas, M. Vaccari, M. W. L. Smith, N. Castro-Rodriguez, N. Lu, N. Rangwala, N. Sacchi, P. Chanial, P. Panuzzo, R. Auld, S. A. Eales, S. Charlot, S. Hony, S. Madden, S. Oliver, S. Srinivasan, T. J. Parkin, V. Buat, W. K. Gear, W. W. Zeilinger","submitted_at":"2010-05-13T14:30:22Z","abstract_excerpt":"We present Herschel-SPIRE observations of the perturbed galaxy NGC4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the galaxy's disk. The dust closely follows the distribution of the stripped atomic and molecular hydrogen, supporting the idea that gas and dust are perturbed in a similar fashion by the cluster environment. Interestingly, the extra-planar dust lacks a warm temperature component when compared to the material still present in the disk, explaining why it was missed by previous far-infrared investigations. 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