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Possibilities for Observations with the Infrared Space Observatory of Emission from Shock–Heated Dust in SNRs
Published online by Cambridge University Press: 12 April 2016
Abstract
The possibilities for observing infrared emission from shock-heated dust in SNRs with the future Infrared Space Observatory (ISO) are illustrated with calculations of the ISOPHOT-P and ISOPHOT-C flux densities and integration times for radiation from six selected SNRs in eight wavelength bands between 4µm and 180µm.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 387 - 390
- Copyright
- Copyright © Cambridge University Press 1988