Abstract
We summarise the properties of selected supernova remnants (SNRs) which have elongated envelopes that could house relativistic jets. We present MOPRA and SEST millimeter observations of these objects, showing correlation between known X-ray hot spots and molecular cloud density as signified by the detection of a CO(l–0) line flux.
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References
Gaensler, B.M.: 1998, Astrophys. J. 493, 781.
Lu, F.J.: 2000, these proceedings.
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© 2001 Springer Science+Business Media New York
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Durouchoux, P. et al. (2001). Elongated SNRs: Possible New Jet Sources. In: Castro-Tirado, A.J., Greiner, J., Paredes, J.M. (eds) Microquasars. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0700-9_38
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DOI: https://doi.org/10.1007/978-94-010-0700-9_38
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3828-7
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