Now showing items 1-4 of 4

    • Infrared polarimetry of the southern massive star-forming region G333.6-0.2 

      Fujiyoshi, T.; Smith, C.H.; Wright, C.M.; Moore, T.J.T.; Aitken, D.; Roche, P.F. (2001)
      We present 8-13μm spectropolarimetry, and 12- and 2-μm imaging polarimetry of the southern massive star-forming region G333.6−0.2. Spectro-polarimetry measurements show that the polarization observed towards the nebula ...
    • Mid-infrared polarimetry and magnetic fields : an observing strategy 

      Aitken, D.; Hough, J.; Roche, P.F.; Smith, C.H.; Wright, C.M. (2004)
      Linear polarimetry in the mid-infrared can be used to obtain magnetic field directions in astronomical sources. However, since the polarization can arise from emission and/or absorption from aligned grains, care is needed ...
    • Mid-IR spectra of type Ia SN 2014J in M82 spanning the first 4 months 

      Telesco, C.M.; Hoflich, P.; Li, D.; Alvarez, C.; Wright, C.M.; Barnes, P.J.; Fernandez, S.; Hough, James; Levenson, N.A.; Marinas, N.; Packham, C.; Pantin, E.; Rebolo, R.; Roche, P.; Zhang, H. (2015-01-10)
      We present a time series of 8-13 μm spectra and photometry for SN 2014J obtained 57, 81, 108, and 137 days after the explosion using CanariCam on the Gran Telescopio Canarias. This is the first mid-IR time series ever ...
    • Studies in mid-infrared spectropolarimetry - II : An atlas of spectra 

      Smith, C.H.; Wright, C.M.; Aitken, D.; Roche, P.F.; Hough, J. (2000)
      We present 8–13 μm spectropolarimetry of 55 sources and 16–22 μm spectropolarimetry of six of these. This represents a substantial fraction of star formation regions that can be observed in this way with current technology ...