Accounting for the foreground contribution to the dust emission towards Kepler's supernova remnant

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Whether or not supernovae contribute significantly to the overall dust budget is a controversial subject. Submillimetre (sub-mm) observations, sensitive to cold dust, have shown an excess at 450 and 850 μm in young remnants Cassiopeia A (Cas A) and Kepler. Some of the sub-mm emission from Cas A has...

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Autores principales: Gomez, H.L., Dunne, L., Ivison, R.J., Reynoso, E.M., Thompson, M.A., Sibthorpe, B., Eales, S.A., Delaney, T.M., Maddox, S., Isaak, K.
Formato: JOUR
Materias:
Galaxies: abundances
ISM: submillimetre dust
Radio lines: ISM
Submillimetre
Supernovae: Kepler
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00358711_v397_n3_p1621_Gomez
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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