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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Prof Patrick Roche

Professor of Physics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
Pat.Roche@physics.ox.ac.uk
Telephone: 01865 (2)83133
Denys Wilkinson Building, room 765
  • About
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  • Publications

10-MU-M AND 20-MU-M SPECTROPOLARIMETRY OF THE BN OBJECT

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 236:4 (1989) 919-927

Authors:

DK AITKEN, CH SMITH, PF ROCHE
More details from the publisher

SPECTROPOLARIMETRY OF THE 3-MU-M ICE FEATURE IN MOLECULAR CLOUDS .2. GL 2591, GL 2136, W33A AND ELIAS 29 (RHO-OPHIUCHI DARK CLOUD)

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 241:1 (1989) 71-88

Authors:

JH HOUGH, DCB WHITTET, S SATO, T YAMASHITA, M TAMURA, T NAGATA, DK AITKEN, PF ROCHE
More details from the publisher

THE EMISSION STRUCTURE BETWEEN 11-MU-M AND 13-MU-M ACROSS THE ORION IONIZATION FRONT

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 236:2 (1989) 485-494

Authors:

PF ROCHE, DK AITKEN, CH SMITH
More details from the publisher

THE NATURE OF THE INFRARED LUMINOUS GALAXIES ARP-220 AND NGC-6240

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 241:3 (1989) 425-431

Authors:

CH SMITH, DK AITKEN, PF ROCHE
More details from the publisher

10 micron spectral observations of SN1987A - The first year

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 235 (1988) 19P-31P-19P-31P

Authors:

DK Aitken, CH Smith, SD James, PF Roche, AR Hyland, PJ McGregor

Abstract:

Spectra of SN1987A in the 10-micron region taken on days 257 and 366-371 after core collapse are presented. The hydrogen/helium envelope is partially ionized at the few percent level and this provides the free-free continuum and hydrogenic lines. There is relative transparency in the midinfrared, while the bound electrons provide the X-ray opacity which is still considerable at day 370. The continuum appears to have become optically thin from about 6 months, and there may be a contribution from low ionization middle mass elements and the iron group. Apart from an excess between 8-9 microns which has been tentatively attributed to molecular SiO, there is no evidence of departure from the emission expected from an optically thin plasma, and no sign of any emission from dust.

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