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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.

Professor Stephen Smartt CBE FRS MRIA

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Hintze Centre for Astrophysical Surveys
  • Pulsars, transients and relativistic astrophysics
  • Rubin-LSST
stephen.smartt@physics.ox.ac.uk
Telephone: 01865273405
Denys Wilkinson Building, room 714
  • About
  • Publications

The VLT-FLAMES survey of massive stars: rotation and nitrogen enrichment as the key to understanding massive star evolution

(2007)

Authors:

I Hunter, I Brott, DJ Lennon, N Langer, PL Dufton, C Trundle, SJ Smartt, A de Koter, CJ Evans, RSI Ryans

A deeper search for the progenitor of the Type Ic supernova 2002ap

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 381:2 (2007) 835-850

Authors:

RM Crockett, SJ Smartt, JJ Eldridge, S Mattila, DR Young, A Pastorello, JR Maund, CR Benn, I Skillen

A very faint core-collapse supernova in M85

(2007)

Authors:

A Pastorello, M Della Valle, SJ Smartt, L Zampieri, S Benetti, E Cappellaro, P Mazzali, F Patat, S Spiro, M Turatto, S Valenti

SN 1996cr: Confirmation of a Luminous Type IIn Supernova in the Circinus Galaxy

AIP Conference Proceedings AIP Publishing 937:1 (2007) 427-429

Authors:

FE Bauer, S Smartt, S Immler, WN Brandt, KW Weiler, Stefan Immler, Kurt Weiler

Abstract:

We have recently confirmed SN 1996cr as a late‐time type IIn supernova (SN) via VLT spectroscopy and isolated its explosion date to ∼1 yr using archival optical imaging. We briefly touch upon here the wealth of optical, X‐ray, and radio archival observations available for this enigmatic source. Due to its relative proximity (3.8±0.6 Mpc), SN 1996cr ranks among the brightest X‐ray and radio SNe ever detected and, as such, may offer powerful insights into the structure and composition of type IIn SNe. We also find that SN 1996cr is matched to GRB 4B 960202 at a 2–3σ confidence level, making it perhaps the third GRB to be significantly associated with a type II SN. We speculate on whether SN 1996cr could be an off‐axis or “failed” GRB.

A very faint core-collapse supernova in M85

Nature Springer Nature 449:7164 (2007) e1-e2

Authors:

A Pastorello, M Della Valle, SJ Smartt, L Zampieri, S Benetti, E Cappellaro, PA Mazzali, F Patat, S Spiro, M Turatto, S Valenti

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