Oxford
Astrophysics
Projects
Marlborough College
Blackett Observatory


MSci Projects

  • More details to follow:

  • Topic : Variable Stars in NGC 188

  • NGC 188 is a circumpolar open cluster containing many stars between R = 15 and R = 19 magnitude. By taking repeated CCD images through a R filter, variable stars can be identified.

  • Sequences of images taken every few minutes over many hours and several nights are compared and the brightness of all stars in the field measured using 2-d photometry software. Approximately 10 variable stars have so far been identified

  • Dr T. Lynas-Grey/Dr I. Lewis