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Interstellar dust

Supernova 1987A observed in different wavebands, credit ALMA/ESA/NASA
Supernova 1987A observed in different wavebands, credit ALMA/ESA/NASA

If it were not for interstellar dust, molecular gas and stars would not exist at all.

Interstellar dust hides half of all the optical light ever emitted by stars and galaxies. However, until only a few years ago it was not even clear where and how this dust was made. Our group has shown that the majority of dust is made in supernovae. With detailed observations of SN 1987A, the closest supernova since the invention of the telescope, we are investigating how dust and molecular gas is made in these titanic explosions.

Professor Haley Gomez

Professor Haley Gomez

Deputy Head of School
Astronomy Group
Cardiff Hub for Astrophysics Research and Technology

Email
gomezh@cardiff.ac.uk
Telephone
+44 (0)29 2087 4058
Dr Mikako Matsuura

Dr Mikako Matsuura

Reader
Astronomy Group
Cardiff Hub for Astrophysics Research and Technology

Email
matsuuram@cardiff.ac.uk
Telephone
+44 (0)2922 510266