The distance and spectrum of 3C 391

Caswell, J. L. ; Dulk, G. A. ; Goss, W. M. ; Radhakrishnan, V. ; Green, A. J. (1971) The distance and spectrum of 3C 391 Astronomy and Astrophysics, 12 . p. 271. ISSN 0004-6361

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The angniar structure and low-frequency spectrum of 3C 391 have been investigated with new high-resolution observations at 80 and 408 MHz. The spectrum has a turnover near 408 MHz. An H I absorption kinematic distance shows that the source is at least < 5 kpo distant. The new data are compatible with the conclusion that 3C 391 is a supernova remnant.

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Deposited On:14 Mar 2012 07:42
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