
Hidden and mysterious. Great swaths of dust disguise this direction in our galaxy. This great molecular cloud harbours the formation of new solar systems. However, facination with the field lies not with what is seen, but instead by the intimated hints of activity. Subtle glows of pink and blue do little to cast warmth on a field that shows the structure of the cold interstellar medium. To the left the cluster and surrounding bluish reflection nebula of IC348 punctuate the darkness. To the right the strange and ornate concentration of NGC 1333 looks as a miniature peacock amid dark and foreboding clouds.
The observations were made by a team of astronomers working at the Laboratoire d'Astrophysique de l'Observatoire de Grenoble (LAOG), France, using the Canada-France-Hawaii Telescope (CFHT). Andrew Burgess will be presenting the discovery at the European Week of Astronomy and Space Science at the University of Hertfordshire, Hatfield, on Wednesday 22nd April.
The dwarfs were found in a star forming region named IC 348, which lies almost 1000 light years from the Solar System towards the constellation of Perseus. This cluster is approximately 3 million years old - extremely young compared to our 4.5 billion year old Sun - which makes it a good location in order to search for the lowest mass brown dwarfs.








