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G54.4–0.3 — Multi-Frequency Investigation of an SNR in Interaction with the ISM

Published online by Cambridge University Press:  25 May 2016

N. Junkes
N. Junkes*
Affiliation:
Institut für Astronomie und Astrophysik, Universität Kiel, D-24098 Kiel, Germany

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G54.4–0.3 is an extended shell-type supernova remnant (SNR) in the Galactic plane. We selected this source as a candidate for the interaction of SNRs with the interstellar medium on the base of an investigation of cool IRAS point sources in the direction of SNRs. We found a statistical excess of IRAS sources with FIR spectra similar to young stellar objects (T d ≈ 25 − 45 K) in the vicinity of G54.4–0.3 and a number of other SNRs in the northern hemisphere (Junkes & Fürst 1992).

Type
Chapter 7: How are we to Understand the Small Scale Structure of the ISM?
Information
Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 627 - 628
Copyright
Copyright © Kluwer 1996 

References

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