![Loading...](https://link.springer.com/static/c4a417b97a76cc2980e3c25e2271af3129e08bbe/images/pdf-preview/spacer.gif)
-
Article
Steep-spectrum radio lobes near the galactic centre
In a previous paper1 we reported the discovery of an extended steep-spectrum radio lobe located ∼34 arc min north-east of the galactic centre (the northern galactic centre lobe). Based on the similarity of the ob...
-
Article
A fast pulsar candidate in the globular cluster M28
Hamilton, Helfand and Becker1 (hereafter termed HHB) have recently used the Very Large Array (VLA) telescope at 1,465 MHz to observe radio sources in globular clusters. These observations were primarily motivated...
-
Article
Observation of highly excited radio recombination lines towards Cassiopeia A
The absorption line at 26 MHz observed by Konovalenko and Sodin1 towards Cas A was interpreted by Blake et al.2 as the 631α recombination line due to carbon or heavier elements. This was confirmed subsequently by...
-
Article
Generation of Polarized Light in the Crab Nebula
IT does not appear to have been noted previously that the polarized light emitted by the Crab Nebula could be generated in an elementary manner. In the collisions between high-velocity clouds of presumably ion...