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Stellar and High-Energy Astrophysics at UBC

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Cool Images

A selection of big images from our research:

  • Dynamics and Mechanics
    • The Double Pendulum Fractal (32757×32736)
  • Globular Clusters with Hubble:
    • The Core of 47 Tuc in the UV (10307×9960 PNG)
    • The Core of NGC362 in the UV (5760×5200 PNG)
    • The Core of Omega Centauri in the UV (7000×7000 PNG)
    • NGC 6397 in the visual through ultraviolet (5284×5096 PNG)
    • NGC 6528 in the visual through near infrared (5284×5096 PNG)
    • NGC 6553 in the visual through near infrared (4270×4243 PNG)
  • Globular Clusters with Gemini
    • Liller 1 in the near infrared (4754×4775 PNG)
    • Liller 1 (single exposure)in the near infrared (4754×4775 PNG)
  • Simulated Images of Globular Clusters for JWST
    • 47 Tuc JWST Simulations from ACS and WFC3 Data
      • A simulated long-exposure in 47 Tucanae (outer field) with JWST (10573×10246)
      • A simulated series of exposures in 47 Tucanae (outer field) with JWST (10573×10246)
      • A simulated image of one quarter of the core of 47 Tuc (10573×10246)
    • JWST Simulations from Measured Luminosity Functions
      • An image simulated using the luminosity function of 47 Tuc and the SMC for 20 square arcminutes and a 5-hour exposure (9714×7814 PNG)
      • An image simulated using the luminosity function of Liller 1 and Galactic Stars for a NIRCAM field and 1.5-hour exposure in F150W and F200W and 3-hours in F444W (liller_jwst.png)
  • Open Clusters:
    • Messier 47 from VPHAS+ data

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Department of Physics and Astronomy
University of British Columbia
6224 Agricultural Road
Vancouver BC V6T 1Z1

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We study stellar astrophysics, neutron stars and black holes with the latest space and ground-based telescopes.

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