HD 35298 is the fifth magnetic B-type star found to emit coherent radio pulses; the pulse pattern identifies the emission mode and implies a dense magnetosphere.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?
HD 35298 is the fifth magnetic B-type star found to emit coherent radio pulses; the pulse pattern identifies the emission mode and implies a dense magnetosphere.