Prof Patrick Roche

Abstract:

Spectra are presented with a resolving power λ/Δλ \ap 1100 of the dusty Wolf-Rayet star Ve 2-45 and the southern H II region G333.6-0.2. An upper limit on the equivalent width of any features in the range 11.0 to 13.0 μm is determined to be 0.0022 μm towards Ve 2-45. This figure is compared with the predicted strength of the unobserved narrow feature at 11.52 μm which has been proposed to be associated with small graphite grains (Draine).

Abstract:

Speckle observations at the peaks of narrow dust emission features at 3.3 and 3.5 microns in the low-excitation planetary nebula CPD-56 deg 8032 and the peculiar emission-line star HD 97048 are presented. In CPD-56 deg 8032 the emission in the 3.28-micron band is extended on a scale of approximately 1.3 arcsec, and this is probably the same as the extent of the ionized nebula. By contrast, the emission in the 3.53-micron band in HD 97048 is spatially unresolved and arises from a region less than 0.1 arcsec across. Dust grains within 0.05 arcsec of the star have temperatures not less than 1000 K, so that the proposed identification of the species emitting the strong 3.43-and 3.53-micron features with formaldehyde ice is untenable, and the materials responsible for the band emission remain unidentified.

Abstract:

The results of 8-13 micron spectropolarimetric observations of Galactic Center sources are presented. All the sources show interstellar polarization due to absorption by aligned silicate grains, and these grains appear to be spatially separated along the line-of-sight from those which produce the polarization at shorter wavelengths. The line of sources IRS 1, 10, 5, and 8 comprising the northern arc all show strong intrinsic polarization due to thermal emission from aligned grains of amorphous silicate-like material. This polarization is very uniform among these sources with position angle closely normal to the line of the arc. It is shown that the data are inconsistent with grain alignment due to streaming, but favor alignment by a strong magnetic field greater than 10 mG directed along and linking the northern arc of sources. A field of this magnitude will have significant influence on the structure and evolution of sources in the Galactic Center. Some possible implications are discussed.

Abstract:

The authors present observations of the nucleus of NGC 4418 which show it to be perhaps the first true infrared galaxy. NGC 4418 was found to be very bright in the infrared by IRAS, and ground-based observations have been employed to investigate the nature of the infrared emission. Optical spectra show little evidence of the luminous infrared core of the galaxy, revealing only stellar absorption features and very weak emission lines. The infrared spectra have a very deep minimum at 9.7 μm, implying a visual extinction of very large50 mag and indicating that the source producing the infrared luminosity is completely obscured in the visible. From the relatively warm IRAS colours, and the non-detection of dust or ionic line emission structure in the 8 - 13 μm spectrum, it is likely that NGC 4418 harbours a very heavily obscured active nucleus.