Title of article :
Dust production in supernovae: the case of Kepler’s SNR
Author/Authors :
E. M. Reynoso، نويسنده , , H. L. Gomez، نويسنده , , L. Dunne، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2009
Abstract :
We compare the submillimetre (submm) emission with the Hi and CO distribution towards Kepler’s supernova remnant (SNR), and conclude that 0.1 to 1.2 M_ of dust originates from Kepler. Such rates are sufficient to explain the origin of dust in high redshift galaxies.
Keywords :
Supernova remnants , individual: Kepler’s SNR , submillimetre , dust
Journal title :
Proceedings of the International Astronomical Union
Journal title :
Proceedings of the International Astronomical Union
